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NATURE 





THURSDAY, JANUARY 22, 1880 


TURUS 
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ON THE PHOTOGRAPHIC SPECTRA OF 
STARS? 
HE author presented, in December, 1876, a preli- 
minary note on the subject of this paper, together 
with a diagram of the spectrum of Vega compared with 
that of the sun. 

The author refers to a paper by Dr. William Allen 
Miller and himself in 1864, in which they describe an 
early attempt to photograph the spectra of stars. 

Other investigations prevented the author from re- 
suming this line of research until 1875, when a more 
perfect driving clock, by Grubb, enabled him to take up 
this work with greater prospect of success. 

The author describes the special apparatus and the 
methods of working which have been employed. 

In consequence of the very limited amount of light 
received from the stars, it was of great importance not to 
spread out the spectrum to a greater extent than was 
necessary for a sufficient separation of the principal lines 
of the spectrum. The spectrum apparatus finally adopted 
consists of one prism of Iceland spar and lenses of 
quartz. The length of the spectrum taken with this appa- 
ratus is about half an inch, from G to O in the ultra-violet. 
The definition is so good that in photographs of the solar 
spectrum at least seven lines can be counted between H 
and K. 

Though there is considerable loss of light in the 
employment of a slit, still, for the great advantage which 
it affords in obtaining spectra of comparison, a narrow 
slit one-three-hundred-and-fiftieth (35) of an inch in 
width was always employed. 

This slit is provided with two shutters. By means of 
these through one half of the slit a solar or other spectrum 
may be taken on the same plate for comparison, and for 
the determination of the lines in position in the spectrum. 
This apparatus was adapted toa Cassegrain reflector with 
a metallic speculum of 18 inches aperture. The small 
mirror was removed and the slit of the spectrum appa- 
ratus placed at the principal focus of the mirror. A 
simple but perfectly successful method was adopted by 
which the image of a star could be brought exactly upon 
the slit, and retained there during the whole time of 
exposure, sometimes for more than one hour, by a system 
of continuous supervision, and instant control by hand 
when necessary. 

Various photographic methods were tried, but the great 
sensitiveness which may be given to gelatine plates, 
together with the special advantages under long exposures 
of dry plates led finally to the exclusive adoption of this 
method. 

The photographs were examined and the lines measured 
by means of a micrometer attached to a microscope of 
low power. These measures were reduced to wave- 
lengths by the help of solar and terrestrial spectra, use 
being made of M. Cornu’s map of the ultra-violet part of 
the spectrum, and of M. Mascart’s determination of the 
wave-lengths of the lines of cadmium. 

Photographs have been obtained of the stars Sirius, 


? Abstract of paper by W. Huggins, D.C.L., LL.D., F.R.S., read before 
the Royal Society, December 18, 1879, with additions by the author. , 


VOL. XXIL—No. 534 


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Map of Photographic Spectra of Seven Stars. 








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270 


NATURE 


[ Fan. 22, 1880 





Vega, a Cygni, a Virginis, » Ursz Majoris, a Aquilz, 
Arcturus, 8 Pegasi, Betelgeux, Capella, a Herculis, Rigel, 
and a Pegasi. Also of the planets Jupiter, Venus, and 
Mars, and of different small areas of the moon. 

The spectra of Sirius, Vega, a Cygni, a Virginis, » Ursze 
Majoris, a Aquilz and Arcturus are laid down in the map 
on the scale of M. Cornu’s map of the ultra-violet part of 
the solar spectrum. 

The stellar spectra extend from about G to O in the 
ultra-violet. 

Six of these spectra belong to stars of the white class. In 
1864 the author pointed out the features in common in the 
visible spectra of these stars. These photographs present a 
remarkable typical spectrum consisting of twelve strong 


lines (seven only of these were given in the preliminary | 


note in 1876). The least refrangible of these is coincident 
with the hydrogen line (y) near G. The second with / 
also a line of hydrogen. The third with H. K if present 
at all, is thin and inconspicuous." 


These lines, H and K, are coincident with lines in the | 





| calcium spectrum, and are usually attributed to the 


vapour of this substance. Now there is another pair of 


| strong lines in the spectrum of calcium, which in M, 


Cornu’s map have the wave-lengths 3736°5 and 3705's. 
There are no strong lines in the white stars coincident 
with these lines. A glance at the map will show how 
remarkable is the arrangement in position of these twelve 
typical lines. They form a great group in which the 
distance between any two adjacent lines is less as the 
refrangibility increases. It is at once suggested that 


| they are connected with each other and represent probably 


one substance, and two at least belong to hydrogen. 

It should be stated that the continuous spectrum ex- 
tends in the photographs beyond S, but no lines can be 
detected beyond the twelfth line at A 3699. For the sake 
of convenience of reference the author distinguishes these 
lines by the letters of the Greek alphabet in the order of 
refrangibility, beginning with the first line beyond K of 
the solar spectrum. The wave-lengths of these lines are 
as follows :— 


Photographic Spectrum of a Lyre. 


Hydrogen 
near 


4340 
4101 
3968 
3887°5 
3834 
3795 
3767°5 
3745 
3730 
3717°5 
3707°5 
3699 


PeEyanPunn 
- O32" OY Da THEO 


10. 
II. 
12. 


In all these stars the line K is either absent or very 
thin as compared with its appearance in the solar spectrum.” 
In the spectrum of Arcturus, which belongs to the solar 
type, this line exceeds in breadth and intensity its con- 


dition in the solar spectrum. The white stars may, 
therefore, be arranged in a series in which the line K 
passes through different stages of thickness, at the same 
time that the typical lines become narrower and more 
defined, and other finer lines present themselves in in- 
creasing numbers. Arcturus seems to present a spectrum 


* The author refers to Mr. Lockyer’s paper, Proceed. R. S., No. 168, 
1876, in which he Suggested that photographs of the spectra of the brighter 
stars might show modifications of this annater of the lines of the calcium 
spectrum, and that such modifications would confirm his views on the 
dissociation of this substance. fe is also made to Proceedings R.S., 
December, 1878, Fig. 1, where Mr. Lockyer gives a fuller statement of his 
views on this and other points in connection with different classes of spectra 
of ~~ stars. 

essrs. Dewar and Livei ve found in their experiments similar 
relative changes of intensity of the lines of calcium corresponding to H and 
K in the emission spectrum of calcium. 








on the other side of that of the sun in the order of changes 
from the white-star group. 

The spectra of the planets were taken on the plan sug- 
gested by the author in 1864, in which the planet’s 
spectrum is observed or photographed together with a 
daylight spectrum. These photographs show no sensible 
planetary modification of the violet and ultra-violet parts 
of the spectrum of the planets Venus, Mars, and Jupiter. 

Numerous spectra of small areas of the lunar surface 
have been taken under different conditions of illumination, 
and during eclipses of that body. The results are wholly 
negative as to any absorptive action of a lunar atmo- 
sphere. 

The author is preparing to attempt to obtain by photo- 
graphy any lines which may exist in the violet and ultra- 
violet spectra of the gaseous nebulz. He also points out 
the suitability of the photographic method of stellar 
spectroscopy, first inaugurated by his researches, to some 
other investigations, such as—differences which may pre- 
sent themselves in the photographic region in the case of 
the variable stars, the difference of relative motion of two 
stars in the line of sight, the sun’s rotation from photo- 
graphic spectra of opposite limbs, and the spectra of the 
different parts of a sun-spot. 

In the hope of throwing light on many physical ques- 
tions suggested by the stellar photographs, the author has 
taken for comparison a number of terrestrial spectra, 
especially of hydrogen and calcium, under different 
physical conditions. As he is still pursuing this inquiry, 
he reserves an account of this part of his work. 





Fan. 22, 1880] 


NATURE 


271 





VOCAL PHYSIOLOGY AND HYGIENE 


A Treatise on Vocal Physiology and Hygiene, with 
Especial Reference to the Cultivation and Preservation 
of the Voice. By Gordon Holmes, L.R.C.P. (Edin- 
burgh: Churchill, 1879.) 

* is one of the most singular facts connected with 

music that, notwithstanding the very wide spread of 
musical education, the kind of performance which is within 
the most general reach, namely, singing, receives the 
least amount of earnest culture. Almost every indi- 
vidual in ordinary health possesses the means of singing, 
which consist simply of a voice that can produce musical 
tones, and an ear that is capable of guiding its inflections. 

The latter qualification is, it is true, not socommon as the 

former ; but in all probability the cases where the human 


pitch are extremely rare, 
mankind what a small proportion actually sing; and of 
those who do, what a still smaller proportion even aim at 
singing well ! 


regard to that small fraction of mankind who attempt 
to sing-in some fashion or other. The great majority of 
these never /earn at all; they sing by the light of nature, 
using their voices in any way that will produce the notes 


their ears guide them to; and, no doubt, with naturally | 


good voices and naturally good ears, music may some- 
times result, which is quite tolerable, though infinitely 
inferior to what it might be made. But many persons 
do “learn to sing,” and instruction of this kind forms a 
tolerably large professional avocation. What, then, does 
this imply? In most cases, unfortunately, little or 
nothing, so far as the true art is concerned. 


ordinary teacher, we know pretty well what will be done: 


there may be, just as a matter of form, a few exercises | 


given; but the great aim will be to teach her the notes of 
certain songs, so as to provide her with a small repertory 
for social exhibition. This, however, is rather teaching 
music than singing, and the same may be said of the large 
number of classes for vocal performance in parts, where 
nothing is attempted beyond attention to the pitch of the 
notes used, and the time they are sung in. If we goa 
little further and include the cases where the teachers en- 
deavour to give their pupils some idea of style, we about 
exhaust the category of vocal instruction which is common 
in private circles, and we need not wonder at the fact 
that, to educated judges, ordinary amateur singing, when 
it is not offensive, is at all events wretchedly poor. To 
learn to sing in the proper sense of the word is quite a 
different thing from learning songs; the voice is an 
instrument, the capabilities of which, in many respects, 
transcend those of any other known, and the cultivation 
of the voice, and of the singer’s power over it, so as to 
use it to the best advantage, requires not only careful and 
judicious training, but long, hard, and laborious practice. 
It is consequently only among the professional ranks 
that we are accustomed to expect thoroughly good singing, 
and even here, whether from deficient education, imperfect 
powers, or defective taste, it is not often that what we 
expect is really found. 

We might extend these remarks, in some measure to 








If a girl who | 
finds she can sing a little asks for some lessons from an | 





speaking. Although the natural use of the voice suffices 
for common practical purposes, there are cases where 
considerable art and education are required to employ it 
to the best advantage, and yet little or no attention is 
paid to the matter, as is evidenced by the miserable 
attempts at untrained elocution we are so often doomed 
to listen to, in preaching, reading, and public speaking. 
The stage is an exception, as there the artistic manage- 
ment of the voice is indispensable, a fact at once perceived 
when amateur acting is compared with that of the members 
of the dramatic profession. 

Undoubtedly one of the great causes of the evil in 
both these cases is the general ignorance as to the nature 
of the voice and the manner in which it admits of 


| management ; and we welcome with pleasure the appear- 
; ance of a work which sets forth these and kindred 
ear is absolutely wanting in the discrimination of musical | 
Yet out of this great mass of | 


topics in a way that cannot fail to be largely useful. 
Although written by a man who is fully conversant with 
all the technicalities of his subject, it is yet essentially 


| popular in its style, and may be studied with advantage by 
| all who are interested in the cultivation of the voice for 
Let us consider for a moment how the case stands in | 


any object whatever. 

The introduction and the first chapter are devoted to 
an Historical Review of the Origin and Progress of Vocal 
Culture, and to an explanation of the general nature of 
musical sounds. These are somewhat lengthy, occupying 
one-fourth of the book; but one may fairly allow for the 
author’s wish to render his treatment of the subject com- 
plete. In the remainder of the work he is more clearly 
on his own ground. Chapter II. is devoted to a descrip- 
tion of the anatomical construction of the vocal organs, 
and Chapter III. to an investigation of their physiological 
mode of action. Both these are admirably treated of, and 
are illustrated, where necessary, by copious figures. The 
author gives, under the latter head, an interesting survey 
of the various theoretical attempts that were made to 
explain the vocal phenomena before the great invention 
of the Jaryngoscope in 1854, by Manuel Garcia, gave the 
power of actually observing the processes at work. By 
the aid of this ingenious apparatus, the explanation be- 
came comparatively easy. There are, however, some 
points, particularly connected with the falsetto voice, 
which are yet somewhat obscure. 

Chapter IV. is the one to which, probably, the greatest 
importance is to be attached ; it treats of ‘‘ The Physio- 
logical Principles cf Vocal Culture.” The author says :— 


“ The cultivation of the voice amongst civilised nations 
has for its object the complementary development of the 
powers of organs which have already attained a high 
degree of perfection in the performance of their functions. 
Through the exertion of influences acting from without, 
and not directly controlled by the will, man proceeds 
instinctively and intuitively as a mere agent to the evolu- 
tion of speech and language. But here, as in many other 
of his relations, beyond a certain point the unerring guide 
of nature leaves or only follows him with a perpetually 
widening interval, and his further advance is made volun- 
tarily and with self-consciousness of his aim. . . . Hen-e 
we may recognise two grades in the employment of the 
voice—the first necessitated by the conditions of social 
life as a means of intercommunion, and the second under- 
taken with a view to the zxsthetic ovservation of the 
listeners. 

“ The technical training of the voice lies immediately 
in the hands of teachers of elocution and singing. €n 





272 


NATURE 


[ Fan. 22, 1880 





their taste and genius, as well as on the aptitude and 
natural vocal gifts of their pupils, depend in the greatest 
measure the success obtained and the perfection of the 
result. But whatever methods be adopted, the base of 


operations is vital organisation and action, of which the | , : : 
Abel in an address as president of the Chemical Section 


of the British Association in 1877, that the comparative 
ease with which triumphs may be won in the field of 
| organic research has led the younger chemists to under- 

estimate the importance of rigorous analytical work by 
| which their science has been built up. 


true apprehension and normal guidance must lead most 
directly and certainly to the desired end.’ 

This, we take it, is the great aim, and the most useful 
tendency of the book, namely, in the first place to make 
known to those who desire to excel, either in singing or 
in elocution, that something more is necessary than they 


can obtain by the mere light of nature; and secondly, to | 


enunciate the important truth that the art of using the 
voice to the best advantage can only be effectively taught 
by the aid of a competent knowledge of the nature and 


capabilities of the natural organ—matters of which great | 


numbers of those who profess to teach have absolutely no 
idea at all. 
is conveyed in this work, both to teachers and learners, 
can scarcely be overrated. It is not possible here to 
enter into details ; suffice it to say that the chapter treats 
fully of vocal force, timbre, compass, and execution ; of 
the modes of development; of the management of respira- 
tion ; of the vibrating elements, the resonance apparatus, 


and the articulation ; and it adds some useful data as to | 
the treatment of that troublesome vocal defect—stam- | 


mering. ; 


The last chapter is devoted to a subject of vital interest | 
to those who have to make public use of the voice, namely, | 
The maintenance of the vocal powers is | 


vocal hygiene. 
a matter of no less importance than their cultivation ; 


but there is much ignorance and misunderstanding on | 


this point, and the advice the author gives, coming as it 
does from one having authority, is most valuable. 
WILLIAM POLE 





THE COPPER-TIN ALLOYS 
Preliminary Investigation of the Properties of the Copper- 

Tin Alloys. A Report, Edited by Prof. R. H. Thurston, 

of a Committee on Metallic Alloys, Presented to the 

United States Board (Washington: Published at the 

Government Printing Office, 1879.) 

T is not a little remarkable that the study of the 

metallic alloys has been so generally neglected. 
Alfred Riche observes that this may in part be due to 
the fact that the characteristics upon which we rely in 
ascertaining the constitution of bodies are usually inap- 
plicable to alloys. It is difficult for instance to determine 
with accuracy such physical constants as their melting 
points, for in many cases molecular rearrangement takes 
place when the alloys are heated, and, again, the properties 
of alloys are often greatly altered by the presence of 
impurities in such small quantities that it is impossible to 
estimate them by the balance. 

Systematic efforts to clear up the obscurities with which 
the structure and nature of alloys are surrounded have, 
however, not been wanting. Thus, not to mention the 
well-known experiments of Hatchett, published in 1803, 
in 1855 Calvert and Johnson communicated to the British 
Association the results of a series of experiments, and 
in 1862 this body requested the late Dr. Matthiessen 
to continue his experiments on the chemical nature of 
alloys, the result being a report which certainly modi_ 


The value, therefore, of such information as | 


| fied the views concerning them that had to that time 
| prevailed. England then has certainly not been behind 
| other countries in actual advance in metallurgical pro- 
| cesses, but it is nevertheless true, as was pointed out by 


With regard to France the researches of Levol and of 
| Alfred Riche will always hold a high place in scientific 
history ; and in Germany there are many classical re- 
searches, such as those of Karsten and of Wertheim. 

The volume before us affords abundant evidence that 
the Americans are not unmindful of the importance of 
metallurgical investigation. It appears that a committee, 
| consisting of Prof. Thurston and Messrs. L. A. Beardslee 
and David Smith, was appointed in 1877 by the Govern- 
ment of the United States, to “assume the charge of a 
series of experiments on the characteristics of alloys,” 
and the first result of their labours is an octavo volume, 
edited by Prof. Thurston, of nearly 600 pages, illustrated 
with photographs of fractures, and plates of curves repre- 
senting the various physical constants of the alloys of 
copper and tin. The committee hope soon to present a 
similar report on the alloys of copper and zinc, and a 
third report on the triple alloys of copper, tin, and zinc 
will follow. They state that ‘‘ the whole field has now 
been explored and the useful alloys are proved to occupy 
but a limited portion of its great extent, and it has now 
been shown that a comparatively narrow band, extending 
| from ordnance bronze on the one side of this triangular 
| territory to Muntz metal on the other, contains all the 
best of the alloys that are generally useful.” 

The necessary researches were conducted in the me- 
chanical laboratory of the Stevens Institute of Technology, 
and the committee trust that this preliminary work will 
prove ‘‘to have been so satisfactorily done that its repe- 
tition may never be required, and that in future attention 
may be confined to matters of detail which have been 
shown to be of most promise.’? The committee did not 
seek to determine the character of chemically pure metal, 
but endeavoured to ascertain the practical value of com- 
mercial metals, melted in the way that is usual in the 
preparation of alloys in the foundry. The purest metals 
that could be obtained in commerce appear, however, to 
have been selected, the greatest care being taken to 
ascertain by a minute analysis the amounts of impurities 
in the metals employed and the composition of the 
twenty-seven alloys forming the subject of the Report. 

After carefully noting the characteristics as to fracture, 
colour, and hardness of each alloy, their resistance to 
transverse stress was examined. Tests by tensile stress 
then follow, and the results agree, in general, very closely 
with those given by transverse stress. The alloys were 
then submitted to torsional stress in a machine devised 
by Prof. Thurston, and, if the autographic strain-diagrams 
given by the machine are compared with the curvés 
representing resistance to transverse and tensile stress, 4 
marked similarity will be evident. Experiments proved 
that the maximum resistance to compression is given by 
the alloy containing 69°84 per cent. of copper, and the 











Fan. 22, 1880] 


NATURE 


273 





minimum by pure tin. A second series of alloys was then 
prepared, the mixtures of the constituent metals being 


made without reference to the chemical equivalents or | 


the atomic weights of the metals, but a constant difference 
of 5 per cent. being maintained between each two alloys 
in the series. An attempt was made to obtain the tem- 
perature of pouring of this series by a well-known calori- 
metric method, but the results, of course, only profess to 
be approximate and relative, as the specific heats of the 
alloys are deduced from the mean specific heats of the 
constituents, and are assumed to be the same in the 
liquid as in the solid state. The numbers given, however, 
differ widely from those usually accepted, the “‘tempera- 
ture of casting’’ of copper, for instance, being given as 
1,909° C., while M. Violle (Comptes Rendus, t. \xxxix. 
p. 702) considers its melting point to be 1,054°C. It is 
probable therefore that the metals were poured at tempe- 
ratures considerably above their points of fusion. The tests 
by transverse stress were repeated on this series of alloys 
and the results led the committee to conclude that they 
“do not seem to corroborate the theory given by some 
writers, that peculiar properties are possessed by alloys 
which are compounded of simple multiples of their atomic 
weights or chemical equivalents. . . . It does appear 
that a certain percentage composition gives a maximum 
strength, and another certain percentage a minimum, but 
neither of these compositions is represented by simple 
multiples of the atomic weights. Besides, there appears 
to be a perfectly regular law of decrease from the maxi- 
mum to the minimum strength which does not seem to 
have any relation to the atomic proportions, but only to 
the percentage composition.”’ 

These conclusions are of the utmost interest and are 
certainly somewhat startling ; it may be well to point out 
therefore incidentally that, since the report 
lished, it has been shown in this country that in the curves 
representing the induction-balance effect and the electrical 
resistance of the tin-copper alloys two critical points are 
occupied by alloys in which the constituent metals are 
combined in the very definite atomic proportions repre- 
sented by the formulze SnCu, and SnCu, respectively. 

In summing up the results, the committee point out 
that the curves of resistance to tensile and torsional stress 
agree very closely, the curve of transverse resistance being 
similar, but the compression-curve is very unlike either of 
the others, the maximum compressive resistance being 
‘* reached by one of the brittle alloys, the tensile strength 
of which is not far from the minimum. It appears, there- 
fore, that the tensile and compressive strengths of the 
alloys are in no way related to each other; that the 
torsional strength is closely proportional to the tensile 
strength, and that the transverse strength may depend, in 
some degree, upon the compressive strength as is indi- 
cated by the approach of some portions of the transverse 
curve to the compression curve, but is much more nearly 
related to the tensile strength, as is shown by the general 
correspondence of the curve of transverse with that of 
tensile strength. From the curves of transverse, tensile, 
and torsional strengths it is seen that the strengths of the 
alloys at the copper end of the series increase rapidly with 
the addition of tin, until about 4 per cent. of tin is reached. 

The specific gravities obtained by the committee are 
corrected for temperature and are reduced to the standard 





was pub- | 





of water of maximum density. The results obtained by 
Mallet, Alfred Riche, and other experimenters are plotted 
side by side, but it is much to be regretted that those of 
the committee are only represented by a mean curve 
which at first sight is rather misleading. 

The appendix to the volume contains several reprints 
of important monographs on alloys. There is also a 
valuable bibliography which might, however, have been 
more complete, and should surely have contained refer- 
ences to such important work as Mallet’s on the density 
of metals in the fluid state, to some of the metallurgical 
researches of Eliot and Storer, and to Knox and Mac- 
gregor’s on the thermo-electric properties of certain alloys. 

Viewing the results as a whole there can be no question 
that metallurgists have reason to be grateful for the col- 
lection of facts which have been so laboriously gathered, 
and we trust it will not seem ungracious to express the 
wish that the work had been undertaken in this country. 

W. CHANDLER ROBERTS 





OUR BOOK SHELF 


The Spiders of Dorset, with an Appendix containing 
Short Descriptions of those British Species not yet 
found in Dorsetshire. By the Rev. O. Pickard- 
Cambridge, M.A., C.M.Z.S., &c. From the Proceed- 
ings of the Dorset Natural History and Antiquarian 
Field Club. Vol. i., pp. 1-235, with Three Plates, 8vo. 
(Sherborne: L. H. Ruegg, 1879.) 


ALTHOUGH this book has been in our hands for several 
months, we have hitherto refrained from noticing it, 
hoping the second volume might come to hand, and thus 
have enabled us to give a more complete analysis. In 
the meantime the importance of the work deserves at 
least a preliminary examination. 

Mr. Pickard-Cambridge’s reputation as an arachnologist 
is a sufficient guarantee that any work written by him 
will be carefully executed. He states that his first idea 


| was simply to give a list of the species found in the 


county in which he has so long been resident. Subse- 
quently it was determined that the work should be mono- 
graphic so far as the Dorsetshire species are concerned. 
It was then found that the species of the county included 
over two-thirds of those that occur in Britain, and it was 
decided to give diagnostic characters of the remainder, 
thus rendering the work a Handbook of British Spiders. 
There was urgent need for such a work. With the 
exception of a semi-popular outline sketch there has been 
nothing claiming to be monographic since the now vener- 
able Mr. Blackwall published his magnificent Ray Society 
Monograph in 1860-63. This work noticed 304 species. 
Mr. Cambridge states that 510 are now known to him as 
British, and that 358 of these have been found in Dorset- 
shire. Considerable discrepancy exists in the nomen- 
clature used as compared with that of Mr. Blackwall. This 
has mainly resulted from the well-known labours of Dr. 
Thorell, who, in his ‘‘Synonyms of European Spiders”’ 
(notable as a work in the English language published in 
Sweden), was the first to bring about tolerable uniformity 
in this respect. But very little inconvenience arises 
therefrom. Mr. Cambridge’s handbook cannot supersede 
Mr. Blackwall’s work with its magnificent coloured plates. 
Both must be in the hands of all students of Araneidea ; 
the former elucidates and supplements the latter. 

Mr. Cambridge commences with a copious “ Introduc- 
tion’’ of forty-two pages, written in a pleasing and popular 
style, so far as is compatible with a due explanation 
of the anatomy, &c., and very readable to all so far as 
his general remarks on the habits, means of capture, 
preservation, &c., are concerned. Some of his remarks 





274 


NATURE 


[ Fan. 22, 1880 





we hope to analyse more particularly hereafter, when we 
have the complete work before us. 

Two important suggestions present themselves to us, 
as tending to render the book more useful. The 
first of these it is now impossible to apply. We 
think it would have been far better had the author 
intercalated the diagnoses of those British species not 
found in Dorsetshire amongst the descriptions of the 
others ; this no doubt would have been done, but for the 
original indecision in the plan of the work. It is not yet 
too late to consider the other suggestion, viz., that a table 
of the family and generic characters be given at the end 
of the second volume. The expression at p. xxxvii. of 
the introduction, to the effect that “the subject of classi- 
fication being practically exemplified in each of the 
ensuing descriptions, need not be further gone into here” 
is not in keeping with the popular aims of the work, and 
is not fair to those students who have not already ac- 
quired a considerable amount of that knowledge possessed 
by the author. 

The three plates are excellent, and in Mr. Cambridge’s 
usual analytical style. The work reflects great credit 
upon the local Society that issues it, which deserves the 
support and hearty thanks of all (we fear but few) who 
are interested in British Spiders, 


Studies on Fermentation; the Diseases of Beer, their 
Causes, and the Means of Preventing them. By L. 
Pasteur, Member of the Institute of France. <A Trans- 
lation, made with the author’s sanction, of ‘‘ Etudes 
sur la Biére,” with Notes, Index, and original Illustra- 
tions by Frank Faulkner and D. Constable Robb, B.A. 
Oxon. (London: Macmillan and Co., 1879.) 


WE thoroughly agree with the following sentence from 
the English edition of Pasteur’s important work: “‘ The 
debt which English brewers owe to M. Pasteur can 
hardly be over-estimated;” but, further than this, we 
believe that the debt which biologists of all countries owe 
to him for his researches is also a very large one, for it is 
by a study of these low and simple forms of life that they 
May expect to learn something of the very beginnings of 
life itself. 

On the appearance of the original work a very elaborate 
notice of it appeared in these pages (NATURE, vol. xix. p. 
216) ; we need, therefore, now only call attention to this 
excellent translation, which contains many notes supple- 
menting the facts mentioned in the original edition, several 
original illustrations, which cannot but be of great value 
in the microscopical study of the changes in the liquids 
with which the brewer has to deal, and an excellent index, 
which immensely facilitates the using of the volume. 

This book may be, in the first place, one of special 
interest to the practical brewer, but it has a nearly equal 
interest for every careful student of nature, and it is so 
clearly written, with all the technical expressions so well 
explained, that we doubt not that the ordinary reader 
who takes it up will not put it on the shelf again without 
a perusal. The chapter on the physiological theory of 
fermentation is one we would specially commend to the 
general reader, to whom it may open up a quite new 
field for thought. 





LETTERS TO THE EDITOR 

[The Editor does not hold himself responsible for opinions expressed 
by his correspondents. Neither can he undertake to return, or 
to correspond with the writers of, rejected manuscripts. No 
notice is taken of anonymous communications. 

[ The Editor urgently — correspondents to keep their letters as 
short as possible. The pressure on his space is so great that it 
is impossible otherwise to ensure the appearance even of com- 
munications containing interesting and novel facts.] 


Ice-Crystals 


_I Do not know whether any satisfactory explanation can be 
given of the different forms assumed by ice-crystals on the 





different substances on which they may be formed. These forms 
are very various. During an intense frost some years ago | 
observed upon the handrail of a wooden bridge a perfect forest 
of ice-crystals very closely resembling the form of ferns, standing 
upright, or rather at right angles with the surface from which 
they sprang, with stems, midribs, and fronds, the only difference 
being the prominence of rectangular arrangements. 

Everyone has seen the variety of forms assumed on window- 
panes, where the crystals do not take erect positions as they did 
in the case last mentioned, but lie flat upon the surface of the 
glass. 

My object, however, now is to direct attention to another 
form assumed by ice-crystals which is comparatively rare, and 
which seems to me to indicate the action of forces of a very 
peculiar kind. 

When frost occurs suddenly as a change from a mild atmo- 
sphere highly saturated with moisture (which is common in the 
climate here), a peculiar form of ice-crystal is often formed upon 
rotten branches lying on the ground under trees, This form is 
that of long silky filaments, from two to three inches long, like 
finely spun glass, These seem to effloresce from the rotten wood, 
and form plumes of the most exquisite delicacy and whiteness, 
often curling towards the ends, and lying over the branch from 
which they spring. 

It is curious that this form of ice-crystal seems never to .be 
attached to any rotten branch of which the bark is unbroken ; 
but whenever the bark upon such branches has been split, 
broken, or exfoliated, then from the exposed ligneous surface 
in certain stages of decay, these lovely plumes of ice rise up, 
pushing their way from underneath the projecting bits of bark, 
then bending round them and curling over them, 

What is it in rotten woody fibre which determines this pecu- 
liar form of the ice-crystal? The phenomenon seems to be due to 
some special ‘‘lines of force” connected with this special mate- 
rial under special conditions. 

During the last two nights we have had sharp frost succeeding 
some very mild and very damp days, In the mornings it ap- 
peared as hoar frost upon the grass, but during the whole day, 
long after all hoar frost had disappeared, there were scattered, 
under all the old woods, shining spots of snowy whiteness, and 
on going up to these one found invariably that they were bits of 
rotten branches, with exfoliated bark, and bearing these peculiar 

lumes. 
. If any of your contributors can give any scientific explanation 
of this phenomenon, they would much oblige. ARGYLL 

Inverary, January 13 


Re-Reversal of Sodium Lines 

THE notice of the Proceedings of the National Academy of 
Science in NATURE, vol. xxi. p. 143, misrepresents, of course 
unintentionally, certain remarks of mine upon ‘‘dark” spectrum 
lines, I have not, and never have had, the slightest doubt that 
the dark lines of the solar spectrum are true absorption lines. 
The lines in question, which 1 am inclined to think may not be 
due to absorption, are only those produced in certain peculiar 
cases. If, for instance, a sodium flame be ‘‘urged,” by in 
creasing the intensity of the flame and the quantity of metallic 
vapour present, each of the two D-lines becomes double, as is 
well known, widening out and showing a dark stripe down the 
centre. Hitherto this dark stripe has been universally ascribed 
to the absorption produced by the envelope of colour-vapour 
surrounding the flame. But if a lime-light be placed behind the 
flame, then, as I have found by repeated experiment, this central 
dark stripe re-reverses, and we have the scdium lines quadruple, 
and dark upon a light ground. The experiment is rather delicate. 
The bead of fused sodium bicarbonate in the flame of a Bunsen 
burner is placed some two inches from the slit of a spectroscope 
of sufficient dispersive power to separate the sodium lines about 
a degree; then the incandescent lime is set four or five inches 
behind the flame, and so as to bring the edge of the shadow of 
the bead just on the slit. , 

Now it seems to me that this re-reversal shows that the dark 
stripe which appeared before the lime-light was placed behind 
the sodium flame, could not have been a mere adsorption-line, 
but must have been due to a real doubling of the line, the 
substitution of ‘wo maxima of radiation for a single one ; I am 
unable to see how, on the contrary supposition, the centre of the 
line should have Jess absorptive power than the two pairs of lines 
which show black when the lime is brought into action. _ 

May I mention in this connection a very pretty experiment 





Fan. 22, 1880] 


NATURE 


275 








which shows that the ordinary dark line is simply due to absorp- 
tion? Put into the spectroscope, in place of the micrometer 
wires, an opaque diaphragm of tinfoil with two narrow slits in it 
at right angles to each other, thus 1. Put the sodium flame 
alone in front of the collimator slit, and by a little management 
one of the bright lines can be brought to shine through the 
vertical slit in the diaphragm, while it can also be seen as a sort 
of star in the horizontal one below. Now bring the lime-light 


behind the flame; the brightness of the vertical slit will at once | 
| them ; and as for his defying any one to prove that the insect dies 


considerably increase, but the horizontal slit below exhibits what 


was before the star, as an intensely dar spot in the midst of the | 


bright continuous streak of colour, showing very strikingly that 
the apparent darkness of the line when no diaphragm is used, 
is a mere effect of contrast. 

The paper referred to in the report as a discussion of ‘‘the 
want of achromatism of the ordinary achromatic object-glass,” 
was a comparison of the secondary spectrum of a glass of the 
usual form and of great excellence, formerly used by me at 
Dartmouth College, with that of the instrument now used here. 
The latter is of the Gauss form, and is found to be decidedly 
superior in its colour corrections, while it is inferior in no other 
respect. C, A. YOUNG 

Princeton, N.Y., January 5 


Death of Captain Cook 


ON reading a paper reprinted from the Afemoirs of the Boston 
Society of Tanaet Hts, vol, i, part 3, entitled “ Notes on 
the Volcanoes of the Hawaiian Islands,” by William T. 
Brigham, A.M., I find at page 370 the following strange 
paragraph : ‘*Starting from the western coast at Kealakeakua 
Bay—the memorable scene of Cook’s punishment—the island 
may be described,” &c. 

With writers accustomed to the correct use of the English 
language, the word punishment infers crime. Its use here by 
Mr. Brigham may be only a bilious outpouring of New England 
puritanism, but as it stands on the face of a grave scientific 
paper, it is a permanent accusation against Capt. Cook, whose 
reputation and memory as one of our greatest navigators and 
geographical discoverers, deserve the reverence of every English- 
man, If there be any charge against Capt. Cook’s reputation or 
moral character, which can justify the slur gratuitously cast upon 
his character by Mr. Brigham, in the above passage, lzt it be 
substantiated by one of his countrymen in your pages or else- 
where, but if there be no grounds on which this grave :lur is 
justifiable, then let it not stand unchallenged by your permitting 
this letter to appear in the pages of NATURE. 

London, January 14 ROBERT MALLET 


Electricity of the Blowpipe ‘‘ Flame” 


I HAVE discovered what I believe to be an important fact, viz., 
that the blue pyrocone produced by the blowpipe from an 
ordinary gas-burner is not merely magnetic, but possesses 
polarity, for its point attracts the north pole of a compass, and 
repels the south pole. W. A. Ross 

Acton House, Acton, W., January 17 


Suicide of Scorpion 

I MUST crave a bit of your space to beg Dr. Hutchinson 
(vide NATURE, vol, xxi. p. 226) to look to facts when he would 
refute anything based upon fac/s, and not trust to inferences. 

My experience concerning scorpion suicide points to the fact 
that the ‘‘ central temperature” of a circle of glowing charcoal 
embers (z.¢, glowing when first placed on the ground in the open 
air, and left to die out gradually), one foot inner diameter, was 
never greatly in excess of the summer heat, often above 40° 
C, in the shade in these parts, and no doubt greater at Peshawar. 
I keep no record of this, but I have just made a circle of glowing 
embers of the size of walnuts, one foot in diameter, on the 
kitchen floor, before the open window, suspending immediately 
a Casella standard in the centre and one inch from the ground, 
and a highly graduated Secretan, two inches from charcoal and 
one inch from the floor, both bulbs free, the result being :— 

Centre.—After three minutes, 49°°50 Cent. ; at five minutes it 
had fallen to 46°, and continued to fall gradually. 

Two inches from charcoal,—The heat declined gradually from 
76° C., to which it rose quickly in the beginning ; general tem- 
perature of kitchen = 15°25 Cent. So much for Dr, Hutchin- 





son’s glowing inference ! which points to little short of stupidity 
on my part. 

The fact is that so far from being cruelly scorched, the scorpions 
I have watched did not appear out of their element, except when 
they tried to escape ; then they quickly receded before burning 
themselves, and it was after many such attempts that they 
‘* pierced their head with their sting and died,” as I have stated. 

As to your correspondent’s theory that ‘‘the Aeat fills the 
scorpion,” it does not follow from the experiments as I conducted 


in consequence of the self-inflicted sting, for my part Iam no 
entomologist, and consequently am unable to make the necessary 
post-mortem examination. I simply state what I saw several 
times with a very good pair of eyes, though not, of course, 
‘*patent double-million-magnifying gas microscopes of extra 
power.” I now confirm the statement, and submit that if Dr. 
Hutchinson’s paternal solicitude for Ais scorpions (which feeling, 
mind, I respect) prevents him making such cruel (?) tests, he 
should be content to doubt, and not pit unsound zx/erences 


| against tangible evidence, much less hurl defiance at the heads of 


practical men, F, GILLMAN 


Prov. Jaen, Linares, Spain, January 12 


The Fertilisers of Alpine Flowers 


A FEw years ago I stated my belief in this journal that lepidoptera 
are far more frequent visitors and fertilisers of flowers, and 
that from this cause by far more flowers are adapted to cross- 
fertilisation by lepidoptera, in the Alps than in the lowland. 
But it was then impossible for me to give a sufficient number of 
facts. Now, therefore, having continued my observations in 
the Alps during six summers, and being about to prepare a de- 
tailed work on ‘‘ Alpine Flowers, their Fertilisation by Insects, 
and their Adaptations to them,” I will here give a statistical 
statement of all visits of insects on flowers which I have 
observed (1) in the lowland, (2) in the Alps generally, (3) 
above the boundary of trees; the numbers under 1 being 
extracted from my work, ‘‘ Die Befruchtung der Blumen durch 
Insekten, &c. ” (Leipzig, 1873). 


Tabular Statement of the Visits of Insects to Flowers, observed by 
myself 





3. Above the 


1. Inthe | 2, In the Alps 
boundary of trees. 


Lowland. generally. 


| 4. Dif- 

. | 

cies of | ferent 
visits to 


insects. | boxcar 
owers. 
| 


| & Dif- 
c i © 
ferent |“ Sp 
visits to 
owers. 


a.§ 
cies of 





134 
930 
519 

1,190 

o 


Coleoptera we ae | > | 83 | 33 | 
Diptera w+. see ose 2 598 | 3 | 1, 210 | 
Hymenoptera... «+. 2,75 183 | 88 
Lepidoptera ...  o 36 220 | 2, 148 | 

| i 


Other insects ... 





| 
Total | 5,232 | 2779 





Hence of 1,000 different visits to flowers (differing either by 
the species of flower or by the species of insect) those by— 





j 
| 2. Inthe |3. Abovethe 
L. Le - | Alps gene- boundary of 
eee i. a trees. 


| 





48°22 
334°65 
186°76 
42831 


2°10 


Coleoptera are 
Diptera ” 
Hymenoptera ,, 
Lepidoptera ,, 
Other insects ,, 


89°66 59 


324°93 
241°95 
371 5° 

2°62 


305°49 
525°7% 
69°77 
9°37 





1000°00 | 1000°00 





Lippstadt, January 10 HERMANN MULLER 


** Ideal” Matter 


In Nature, vol. xxi. p. 185, you published a letter from 
Herr v. Nudeln, in which he alluded to the researches of Pro- 





276 NATURE 


[ Fan. 22, 1880 





fessors Hans and Lobwirmski respecting ideal matter of various 
degrees. Can you inform me whether any English publications 
have appeared on this subject, and if not, what foreign works 
would be best suited to give an insight of the results that have 
been arrived at to one who can devote but a limited time to such 
investigations ? > 

Surely the conclusion suggested by your correspondent (viz., 
that the moon in its composition closely resembles caseine) is 
intended only as a joke ; for, assuming the equation given, 

M = C,,N,0,H,, 

and even granting that the quantities m fg are in such propor- 
tion as to make the right-hand member of the above equation 
assume the form of the chemical formula for caseine, there is 
surely no reason why the mass of the moon (which your corre- 
spondent has chosen to denote by C) should be interpreted as 
carbon, nor its direction of motion N as nitrogen, nor its velocity 
O as oxygen, Percy R, HARRISON 


Sun-Spots 


In the ‘‘ Life of Charlemagne,” written by Eginardus, one of 
the Emperor’s household, and afterwards Abbot of St. Bavon’s, 
in Ghent, occurs the following passage :— 

** Per tres continuos viteque termino proximos annos et solis 
et lunz creberrima defectio, ac in sole macula quedam atri 
coloris septem dierum spatio visa.” 

‘*In three successive years nearest to his death [there were] very 
frequent eclipses of the sun and moon, and in the sun there were 
seen certain spots of a black colour, for the space of seven days.” 

This life, written between 814 and 843, and referred to by the 
writer’s contemporaries, has been collated with several MSS. 
by the Bollandists, who givé it in full in their Acta Sanctorum 
under January 28. It is a curious, if not a valuable, contribu- 
tion to the early history of sun-spots, and suggests questions 
which some of your correspondents may care to consider. 

HENRY BEDFORD 

All Hallows College, Dublin, January 15 


A Clever Spider 


IN a letter I have just received from my brother at Ronde- 
bosch, near Cape Town, he narrates the following, which I 
thought might interest some of the readers of NATURE :— 

** On Friday I was much interested in watching a spider and 
male glow-worm, The spider was a common long-legged house 
spider who had a web in the corner of the room. It was an 
aristocratic spider, in fact. Presently a male glow-worm flew 
into the web, and in a few minutes the spider had wound him 
round and round till no Egyptian mummy was more securely 
housed, Just as this operation was being finished, a second 
glow-worm flew into the web, a dong way from the first. Off 
goes the spider, and soon he, too, was encased in silk. Then I 
noticed that the spider went three times backwards and forwards 
between the head of glow-worm No. 2 and a main strand of his 
web, After this he went round cutting all the threads around 
the glow-worm until it hung by the head strands alone. The 
spider then fixed a thread to the tail end, and by it dragged the 
carcase in the direction of glow-worm No. 1 (presumably the 
larder). As soon as the rope attached to the head was taut, the 
spider made the rope he was pulling by fast to a strand of the 
web, went back, cut the head ropes, attached himself to the 
head, and pulled the body towards the larder, until the tail rope 
was taut. In this way, by alternately cutting the head and tail 
ropes and dragging the glow-worm bit by bit, he conveyed it to 
the larder, where it hung alongsde mummy No.1. Another 
presently flew in. After ‘he was enwrapped in silk, the spider, 
whether on purpose or not I cannot. say, cut the last thread by 
which he hung, and dropped him to the ground. Whether he 
thought that this morsel might get ‘high’ before he could eat 
it I cannot say, I should say that the prey was some twenty 
times the weight of the captor.” Li, A. MoRGAN 

St. Thomas’s Hospital, Westminster, January 12 


Erratum in Paper on Tidal Friction 


AN erratum has been pointed out to me in my article in 
NATURE, vol. xxi. p, 235, and I should be glad to correct it. 





The forty-second line of the second column of p, 236 rans :— 
‘* so that the earth will rotate faster than the moon revolves.” 
By a slip of the pen I here wrote ‘‘faster” instead of 
** slower.” G. H. DARWIN 
January 16 





AFGHAN ETHNOLOGY 


‘THE events now in progress on the north-western 

frontier of British India have for the third time in 
this century directed the serious attention of statesmen, 
historians, and ethnologists to the remarkable people 
who give their name, or rather one of their names, to the 
north-eastern division of the Iranian table-land. During 
the empire of the Sassanides the whole of this region, 
from Persia proper to the right bank of the Indus and 
from the Koh-i-Baba, Ghor and other western continua- 
tions of the Hindu-Kiish to the Arabian Sea was known 
as Khorasan, that is, Khoristan, the Land of the Sun or 
the East. This term, with the gradual reduction of the 
Persian sway, has shrunk to the proportions of a province 
on the north-eastern frontier of the Shah’s estates, and 
has been replaced further east by the ethnical expressions 
Afghanistan and Balochistan, the lands of the Afghans 
and Baloches. But these expressions, as so frequently 
happens, are so far misnomers and deceiving that the 
lands in question harbour many other peoples besides 
those from whom they are now named. In Balochistan, 
for instance, the most numerous, powerful, and influential 
element is not the Baloch at all, but the still unfathomed 
Brahfii, from which circumstance it has even been 
suggested that the country ought rather to be called 
Brahuistan. A similar suggestion could not certainly 
well be made with regard to Afghanistan, for here there 
is no other people who can for a moment compare with 
the Afghans in numbers or political importance. Still 
the subjoined rough estimate of the population according 
to nationalities will show that it is very far from being 
homogeneous :— 


Tranian stock ... 
Iranian stock ... 


3,520,000 
1,000,000 


Afghans and Pathans 
Tajiks sce anton 
Hindkis ... .. ... Hindu stock ... 500,000 


Mongolo-Tatar stock 600,000 
Kataghans Tirki stock ... .... 200,000 
Badakshis 4 .- Galcha stock... ... 100,000 
Baloches ... ... ... «. Iranianstock... ... 100,000 
Kizl-Bashes ... ... ... Tirkistock ... ... 75,000 
Kohistanis and Siah Posh Galchastock ... ... 50,000, 


Hazaras and Aimaks 


6,145,000! 


It will be noticed that in this table are included all the 
races forming part of the present Afghan political system 
taken in its widest sense, whose northern frontier is now 
marked by the upper course of the Oxus. Before dealing 
with the Afghans proper, with whom we are chiefly 
concerned, a few words may be devoted to each of the 
minor elements, all of whom continue to keep aloof from 
their neighbours, seldom or never intermarrying, and 
mostly retaining their own national customs, dress, 
religion, and speech. No general amalgamation has, in 
fact, yet taken place of these heterogeneous ingredients, 
so that we cannot speak of the Afghan in the same sense 
as we do of, for instance, the Italian, French, or English 
nations. The Afghan race, though by far the most nume- 
rous, has been politically predominant only since the death 
of Nadir Shah (1747), and its rule has been far too 
checquered by intestine strife and foreign troubles to have 
allowed time or opportunity for the slow process of 


* This figure exceeds by about a million that usually given as the total 


population of Afghanistan. But recent exploration has shown that many of 
than had been 


= tribes ry more numerous _7 iy , and as our 
owledge o! country increases, it wi to contain 
even a gronter population than thas hore gives” 


- A hh Ff Hh So eet oO 





Fan. 22, 1880] 


NATURE 


277 





absorption to have made any perceptible progress. Next 
to them by far the most important are— ) 

The Tajiks, who, here, as elsewhere in Central Asia, 
represent the old civilised Iranian communities, co- 
extensive with the former limits of the Persian empire, 
but since the ascendency of the Tarki, Mughal, Afghan, 
and Brahui races, now forming politically the subject, 
socially the settled, trading, an agricultural elements in 
these regions. Persian, or some variety of it, is still 
everywhere their mother-tongue ; hence, in Afghanistan 
they are collectively known either as Parsivan, z.¢. Persian- 
speaking, or Dehgan, .e. peasants or agriculturists. “The 
Tajiks are Iranians, a remnant of the old Persian popula- 
lation subdued by the Afghans, but still speaking Persian 
and retaining the Persian type of features” (F. von Stein, 
in Petermann’s Mittheilungen for March, 1879); religion, 
Sunnite. Remotely allied to them are— 

The Hindkis, of Hindu stock, who have been long 
settled here chiefly as traders, forming numerous commu- 
nities, especially in the eastern districts, said to be mostly 
of the Shatri caste; religion Brahminical, speech 
Hindustani. 

The Hazaras and Aimaks, occupying the northern 
highlands between Bamian and Herat, the former in the 
east, the latter in the west, are undoubtedly of Mongolo- 
Tatar stock, though now speaking rude Persian dialects. 
They claim descent, some from the Toghiani Tiirks, some 
from the Koreish Arabs, others from the old Kibti race, 
but seem really to be military colonists settled here by 
Jinghis Khan, Manku KhAn, and Timfir. The Aimaks 
(the term simply means horde, tribe, clan), are of the 
Sunni, the Hazaras of the Shiah sect, and are conse- 
quently fiercely opposed to each other. Owing to this 
circumstance they have often been regarded as of different 
races, but “there seems no reason to doubt that the 
Aimaks and Hazaras are the same people, though sepa- 
rated ... by the different sects they have adopted” 
(Col. C. M. MacGregor, “ Afghanistan,’’ p. 246); type, 
high cheek bones, with small grey eyes, scant beard, and 
low stature. The Aimaks occupy the Ghér highlands, 
which must have been almost uninhabited when they 
settled there, for we read in the National Chronicle that 
about I190 A.D., Sultan Shéhab-ed-din removed all the 
Afghan tribes from the Ghér to the Ghazni highlands, 
“in order to become the bulwarks of the seat of empire 
and hold in awe the infidels of Hindustan.’’ Of the 
Aimaks there are four main divisions, the so-called 
“Char Aimak”’ (“ Four Hordes’’) : Taemfiris, Taemiinis, 
Hazara-Zeidnats, and Suris, with a total population, 
according to some authorities, of about 450,000, including 
those now settled in Khorassan. The Hazaras, numbering 
at least 150,000, occupy the region stretching for 250 
miles west from K4bulistan, and are divided into thirty- 
eight main branches with numerous subdivisions, under 
chiefs bearing various titles, such as Khan, Sultan, 
Ikhtiar, Vali, Mir, Mettar, and Turkhan, and hitherto 
practically independent of the DurAni Amirs. Akin to 
them are— 

The Kataghans, a main branch of the Uzbeks, forming 
the bulk of the population in Kunduz and Balkh, that is, 
the region now known as Afghan Turkestan, stretching 
from the northern slopes of the Hindu-Kfish to the left 
bank of the Upper Oxus. They take their name from a 
legendary Kata, from whom they claim descent in two 
main streams, the Beth-bula and Cheguna, with five and 
eleven sub-divisions respectively, each named after one of 
Kata’s sixteen sons. Most of the tribes occupy the 
country south of the Oxus, but 7,000 families are now 
settled north of that river, consequently in Bokhara 
territory; religion Sunnite, speech Tirki; type, small 
stature, broad face, high cheek bones, sparse beard, small 
oblique eyes. Are now mostly settled agriculturists and 

e 


rs. 
The Badakhshis, or natives of Badakhshan, in the 





| 
extreme north-east, beyond Kunduz, and abutting on the 


Pamir table-land, are a pure Aryan race, intermediate 
between the Iranians and Hindus, and of the same stock 
as the highland Tajiks, whom Ch. de Ujfalvy groups 
under the collective name of Galchas,' Chief divisions, 
Darwazi, Roshani, Shugnani, and Wakhi, or WakhAni; 
religion Sunnite, speech Aryan, with Persian and Indian 
affinities. The Wakhi is a distinct variety, retaining 
many old Sanskritic elements, hence R. Shaw thinks it 
may be 4a relic of a primitive organic Aryan language 
current here before the race issued from the Pamir, or 
divided into Vedic and Zendic. It would be interesting 
to compare it with the Jagnéb, which de Ujfalvy tells us 
is unintelligible to the other Galcha tribes of Fergh4na. 
A Galcha skull which has found its way to Paris, has 
been examined by P. Topinard, who pronounces it to be 
identical with those of the early Keltic Aryans, If their 
speech also should prove to be of an organic Aryan type, 
as constituted previous to the dispersion, de Ujfalvy’s 
view might be unreservedly accepted that “Ces pays 
mystérieux recélent sans doute le secret de l’origine de 
notre race.” ? 

The Baloches, of Iranian stock, and regarded by the 
Afghans as their brethren, are represented in Afghanistan 
chiefly by a number of hill tribes in the south-east corner, 
and by some nomads in the south and west along the 
Lower Helmand. Most of them belong to the Rind 
section of the Baloch race, the more important being 
the— 

Kasranis and Bozdars, on north-west border of Dera 
Ghazi Khan: numerous sub-divisions, the Bozdars alone 
with sixty-four septs (Major Minchin), 

Khosahs, south of Sanghar Pass towards Shikarpur ; 
four divisions: Kalulani, Bakiani, Toniani, Sariani. 

Lagharis, overlooking the Sakhi-Sawar Pass, Dera 
Ghazi frontier ; four divisions: Aliani, Hadiani, Boglani, 
Habtiani ; fifty-six sub-divisions. 

Gurchinis, south of the Lagharis, about Chachar Pass. 

Maris, Sham district, east, north, and north-west of 
Kachi; four divisions: Ghazani, Loharani, Bijarani, 
Mazarani; twenty-two sub-divisions. The Mazarani 
have separated from the rest, and are now settled west 
of Sebi and north of the Bolan Pass, 

Rigtis, south of the Maris; two divisions: Firozani, 
Zarkani ; thirteen sub-divisions. 

Kayanis, Seistan, former rulers of that country; by 
some said not to be Baloches, but Kakar Afghans. 

Religion, Sunnite; speech, a rude, uncultivated variety 
of the old Persian; type, regular Caucasian features, 
light or brown complexion; hair often chestnut and even 
fair; eyes light grey and sometimes blue, especially in 
centre and north. Of the many forms of the national 
name, Baloch, Biloch, Beliich, Balfich, Bilich, &c., Ba- 
loch is the best, coming nearest to the true pronun- 
ciation, as Pottinger assured his French translator, M. 
Eyriés. 

The Kisl-Bashes, or “Red Heads,” known collectively 
as Gholam-Khani or Gholam-i-Shah, “servants of the 
King,” are of Tirki stock, and have been settled in 
Herat, the Gulkoh Mountains, but chiefly in Kabul since 
the time of NadirShah. The term was originally applied 
by Shah Ismail to the Nikalu, Jaw4nsher, and four other 
trusty Tarki tribes to whom he owed his successes. But 
since then they have become a sort of brotherhood “much 
akin to the Beyyadiyah or ‘ White Boys’ of Oman, and 
bearing some analogy tothe Mormons” (W. G. Palgrave, 
“Report on Province Trebizond,” 1868). Those of Kabul 
form three divisions: the Jawansher, originally from 
Shisha, the Afshar, Nadir Shah’s tribe, and the Morad 
Khani, composed of all the other Tirkis who have from 


t “ Le-Badakch4n est également habité en grande partie par des Tadjiks 
montagnards ” (Budi. de la Soc. de Géo., March, 1879, p. 250). But Robt. 
Shaw (“High Tartary”) says that physically they approa ch nearer to 
Kashmuirians and other Aryans of Northern India. i borne out by 
their speech, which is more akin to the Sanskritic than to the Iranic family. 

® Loc. cit, p. 252. 





NATURE 


[ Fan. 22, 1880 





time to time removed from Persia to K4bul ; religion, 
Shiah, with secret rites; speech, Persian, and amongst 
themselves, Tirki ; are a very fine race, very fair, with 
an evident mixture of Iranian ard Tatar blood. 

The Kohistanis and Siah Posh (“ Highlanders”’ and 
“Black Clothes ’’) forming the bulk of the population in 
Kohistan, Swat, Kafiristan, Chitral, and generally of the 
southern slopes of the Hindu-Kiish down to the left bank 
of the Kibul river, are of pure Aryan stock, allied to the 
Kashmirians, but probably more closely to the Badakhshis 
and Wakhis. The Kohistanis are Moslem, the Siah Posh 
still mostly pagans, hence called K4firs, or Infidels, by 
their neighbours, and their country Kafiristan. Their 
speech, of which there are ten distinct varieties (Major 
Tanner), is described as neo-Sanskritic, akin to Dardu 
and Lughmani. But it has never been critically studied, 
and may possibly prove to be pre- rather than neo- 
Sanskritic ; is in any case of great philological interest, 
having been isolated from the kindred tongues since the 
eruption of Islim in the tenth century ; type, regular 
features, blue and dark eyes, hair varying from light 
brown to black, broad open forehead, tall and well-made. 
But General A. Abbot (“ Correspondence,” edited by C. 
R. Low, 1879) distinguishes between a fair type with blue 
eyes, the aristocracy “descended of the Greeks’’(?) and 
a very dark type, the aborigines. The Kohistanis north 
and north-west of Kabul, C. R. Markham says, are mainly 
Tajiks (Proc. Geo. Soc., February 2, 1879, p. 117); but 
they are more probably of the kindred Galcha stock, for 
those of Swat are represented as closely akin to the Siah 
Posh whom I take to be of this race. They form two 
main sections, the Torwals and Garwis. They took a 
large share in the recent events about KAbul and have 
just been reduced by the British. The Safis, who have 
also lately been heard of in the same neighbourhood, are 
simply Siah Posh converts of the Tagao valley, Kunar 
district, north of Kabul ; three divisions : Wadin, Gorbaz, 
and Miisawid ; speech Pashae, closcly allied to Lughmani 
and Kohistani of Swat. 

We come now to the Afghans proper, whose original 
home seems to have been the K4bul valley, whence they 
spread westwards to the Ghér country, southwards to the 
Suleiman mountains, and more recently down the Hel- 
mand and Arghandab valleys to Kandahar.’ They call 
themselves Bani-Israel, ‘‘ Sons of Israel,” claiming descent 
either from Saul or from the ten tribes, for on this point 
they do not seem to be quite clear. But this is of the 
less consequence that both claims are alike inadmissible. 
Notwithstanding a certain Jewish expression, which they 
have in common with the Armenians and other races of 
the Iranian plateau, they are beyond all doubt an Aryan 
and not a Semitic race, so far as these terms can be at all 
used as racial rather than linguistic designations. And 
here it may be well to remember that both Aryan and 
Semite belong equally to one ethnical stock, convention- 
ally known to anthropologists as the Caucasian or Medi- 
terranean, and that they can often be distinguished one 
from the other only by the test of language. We have 
the same phenomenon in Europe, where but for their 
speech no one would ever suspect that the Basques of the 
western Pyrenees were other than a somewhat favourable 
specimen of the Aryan race. This test, however, is 
abundantly sufficient to sever them from that connection, 
and the same test must suffice to remove the Afghans 
from the Semitic to the Aryan group. 

Their most general and apparently oldest national 
name is Pukhitin or Pakhtiin, as it is pronounced by the 
Khaibaris, and which has been identified with the mdxrves, 
of whom Herodotus heard through Scylax (509 B.C.) as 
situated about the junction of the Képhes (KA4bul) and 


* Till the time of Sultan Babur, founder of the Mughal empire (beginning 
of sixteenth century) the Afghan language was still confined to the north- 
eastern and western highlands, Persian being e!sewhere current, as it still is 
mostly in the lowlands. 





Indus. Their country they still call Pukhtin-khwa, which 
is equivalent to Watan-khwa, or “Home Land’’; their 
language is always called by them the Pukhti, softened 
in the west to Pushtd, and from Pakhtdna, the plural of 
Pakhtfin, comes the form Pathan by which they are 
known throughout India. This word has been ccnnected 
with the root Pukhta, a hill, so that Pukhtun would mean 
Highlander. But such derivations are seldom trustworthy, 
and it may be questioned whether any people have ever 
called themselves A/z//-men, though often enough so 
named by their neighbours. 

The alternative national name, Afgb4n, by which they 
are exclusively known in Persia and Europe, has been 
regarded by some as synonymous with Pukhtfin, both 
meaning “set free;” but by others it has been con- 
nected with Acvakan, the Agvaka, or “ Horsemen,” of 
the Mahabh4rata, who are supposed to be the Assakani, 
or Assekenes, of the later Greek historians. The natives 
themselves draw a distinction between the two names, 
so that although all Afghans are Pukhtana, not all 
Pukht4na are true Afghans. The latter term is properly 
restricted to the descendants of a legendary Kais, 
one of the first apostles of Islam (ob. 662), from 
whom, through his three sons, Saraban, Batan, and 
Gurgiisht, are supposed to spring the 277 Afghan 
khels (tribes) proper. Of non-Afghan khels there are 
reckoned 128, making 405 Pukhtana khels altogether. Cf 
these 105 are Sarabdni(from Saraban), 77 from Batan, in 
two divisions ; Batanai 25, and Matti 52, these last being 
known as Ghilzae; 223 from Gurgisht, also in two divi- 
sions; Gurgfishtai 95, and Karalanai 128, these last being 
the non-Afghan or Pukhtana khels as above. In this 
traditional account of the national genealogies the distinc- 
tion between the true Afghan and non-Afghan tribes is 
already obscured, for the latter are made to descend from 
Gurgtisht, one of the three sons of Kais, who is elsewhere 
represented as the ancestor of the true Afghans alone. 
But the confusion becomes intensified when it is added 
that the very word Pathan, specially applicable to the 
non-Afghans, and which we have seen is merely the 
Indian form of Pakhtana, is explained to be a cor- 
ruption of Pihtan, ‘rudder,’’ a title said to have been 
conferred on Kais by the Prophet himself. Altogether 
the distinction, though still maintained and recognised 
by the various sections of the people, cannot at all 
be regarded as racial. ‘The true Afghans occupy mainly 
the western, central, and north-eastern districts— Herat, 
Seistan, Kandahar, and the Kabul basin, as far east 
as Peshdwar. The non-Afghans, or Pathans proper, are 
found almost exclusively in the Sufed-Koh and Suleiman 
highlands, as far south as the Kaura or Vahii Pass, 
opposite Dera Fatah Khan. A line drawn from about 
the parallel of Multdn, through this point, westwards to 
Tal through the middle of the Derajat, will very nearly 
form the boundary in this direction of the Pathans on the 
north, and the Baloches and Brahuis on the south. This 
relative geographical area suggests a possible explanation 
of the distinction between the two great divisions of the 
race. From their more westerly position it is obvious 
that the true Afghans must have been the first to adopt 
Islam, and they may have thus come to look upon their 
pagan brethren of the Suleiman highlands as Kafirs, 
undeserving to rank as genuine Afghans, the distinction 
thus originated naturally surviving their subsequent 
conversion. : 

In the subjoined table an attempt is made to give, for 
probably the first time, a complete classification of all 
the main sections of both divisions, with their chief sub- 
branches, approximate number of khels, geographical 
area, and population. The difficulty of the subject, oc- 
casioned mainly by the minute tribal sub-divisions, may 
be concluded from the fact that a complete genealogical 
tree of, say, the Afridis or the Vaziris alone, would occupy 
about two pages of NATURE. 





Fan. 22, 1880] 


NATURE 


279 





TABLE OF AFGHAN AND PATHAN TRIBES. 





Main Sections, 


Chief Subdivisions. 


Total No. 
| of Khels. 





I. 
Durani or Abdali 


II, 
Khugiani... 


III. 
Ghilzae or Ghilji 


IV. 
Visafzae .. 


tenons or Mah- 


mandzae 


VI. 
Kakars 


VII. 
Khataks ... 


VIII. 
Utman Khel ... 


IX, 
Bangash ... 


Afridis 


XI. 


4 
4 


{| 
sot 
}| 
S| 


) 


f 


j 


Orakzaeor Wurukzae | 


‘a 


Shinwaris or Shan- 


waris 


XIII. 
Tirdes 


XIV. 


Jaduns or Gaduns .. 


XV. 
Tarins 


XVI. 
Povindahs 


XVII. 


Vaziris or Waziris ... 


XVIIL 


Shiranis .., 


XIX, 
MG ec digg 


a4 


| 


| 
| 
| 
| 
| 
| 
| 
| 


} 
| 


ay 


} 


as) 


\ 


“| 


f 


oS 


| 2. Bhran : — Chin, 


1. Zirak:—Popalzae, _ Ali- 


kiozae, Barakzae 


2. Panjpao :—Murzae, Alizae, | 


Ishakzae 


Vaziri ; Khairbiin ; Sherzad 


1. Turan :—Ohtak, Sakzae, 


Tunzae 
Chalo, 
Zabar, Ali, Suliman 


1. Mandan :—Usman, Utman 
2. Ysaf:—Isa, Ilias, Mali, 
Rani 


Tarakzae; Halim; Baizae; 


Khwai; Utmin 


Jala ; 
Khidar ; Abdula 


Tari; Taraki; Bolak 


Asil; Shamo; Mandal; Ali 


Miranzae; Baizae; Samalzae 


Kuki; 
Kamr ; 


Malikdin ; Kambar ; 
Zakha; Aka 


Daolat ; 
mail ; 


Utman ; Sipah ; Ish- 
Rabia ; Isa 


Sangu; Ali Sher ; 
Babur; Lohargae 


Sipai ; 


Shibdwani ; Seh Pat 


Salar; Matkhwa; Mansur 


Spin :—Shadi, Marpani, Las- 
rani 


i 
Tor :—Bateh, Haikal, Mali 


Lohani; Nasar; Niazi; Dao- | 


tani; Kharoti; Miani 


|| 1, Utman :—-Mahmud, Ibrahim | 


- Ahmad :—Shin, Sirki, Umur| 


. Mahsud : —Ali, Shahman 
. Gurbaz; 5. Lali 


. Chua :—Yahia, Bairam 
. Sen :—Ahmad, Yahia 
. Uba:—Ahmad, Manu 


| Mahsud; Bahbdadin ; 
Ahmad ; Mardan 


Musa; Kadi; Usman; | 


Musa; | 





Geographical Position. 





Mainly in the tract between Herat and Kandahar, 
400 miles long, 80 to 150 broad; also in 
Ka4bulistan. 


Chiefly in the Jalalabad district, between Surk-db 
and Kabul rivers. Seem to have been originally 
a branch of the Panjpao Duranis. 


In the country bounded N. by the Kabul river, 
E. by the Suleiman Mts., W. by the Gulkoh 
Mts., S. by Khalat-i-Ghilzae and Poti; 3co 
miles long, tco miles broad. A branch at 
Khubes and Nurmanshahr, Persia. 


The hills N. of Peshawar district and in the 
Yusafzae division of the Peshawar district. 


The hills N.W. of Peshawar between Kabul and 
Swat rivers ; chief town Lalpiira. 


Extreme S.E. corner Afghanistan proper. 


S.E. 
Kohat ; 


part Peshawar district, and S. and E. of 


The hills N. of Peshawar between the Mohmands 
and Yiis cafzaes, 


Miranzae, Kohat, and Kiiram valleys ; said to be 


originally from Seistan. 


Lower and easternmost spurs Sufed Koh Mts., 
W. and S. of the Peshawar district, with Bara 
valley and parts of Chura and Tira valleys, 

. and W. 


The Tira highlands, N of Kohat. 


Parts of Khaibar Mts., E. valleys of Sufed Koh 
and on borders of Bajawar. 


Note.—X., XI., and XII. are collectively known 
as the Xhaibaris. 


In the Kot valley of the Shinwari country, but 
distinct from them, 


S. side Mahaban Mts. and Hazara district, 


Peshawar ; said to be Kakars originally, though | 


now with the Yisafzaes. 


N. frontier Biloch province Kachi. 


From head of Gomal S. to head of Lora river 
along W. Suleiman range, their territory form- | 


ing a triangle hemmed in between the Ghilzaes, 
Vaziris and Kakars. 


° 


Suleiman Mts. from Thal to Gomal Pass, 30°-32 
N, lat. 


Suleiman Mts. from the Shekh Hidar Pass 


southwards to the Ramak, 


In the Koh-i-Daman of the Dera I-hmail district, 
opposite the Sangao and Dahina Passes; same 
stock as the Shiranis. 


some also now amongst the Yusafzaes, | 





A branch now with the Khugianis ([I.) | 


Population. 


809,000 





NATURE 


[ Fan. 22, 1880 





TABLE OF AFGHAN AND PATHAN TRIBES (Continued), 








Main Secticns. Chief Subdivisions. 


—— Nee a —_ — 
XX. Gundi; Ali; Mula; Mastu; . 
he Firoz; Maru 5 





Maidan; Danni; Isteah; Al- 
garh; Ada; Lehwanni; 
Ali; Ahmed; Bian, 
Shamu 


XXII 1. Khwaidad :—Babakar, Hasn 
Zaemikhts ° 2. Mahamad :—Wati, Manatu, | 
Mandan 


XXIII. )' 1. Zapi :—Haidar, Idak 
Dawaris ... ... ...) | 2. Ala/di :—Darpa, Amzani 





XXIV. | Ishmail; Matin; Mandu; 
Khostwals ... ...§ Shamal | 


XXV Lajhwar :—Fattakeh, Agar, } 
is... Andaz, Miral, Khajuri, | 
Mangals... ... ... | Za Miral, ajuri | 


XXVI. = 
Jadrans?... 
1. Gagal :—Shaho, Musa, 
XXVII. Ako, Shamo 
Ushtaranas ... ) | 2. Ahmad:—Tbrahim, Kadr, 
Mashar 


| 1. Moh :—Ahmad, Zado, Ja- 
XXVIII. han, Chado 
I ee 2, Mila :—Ado, Khidr, Pain- 
da, Khadi 


XXIX, Ramdani; Mohra; Rajali; 
re Rawani 


1,790 





| Total No. 
| of Khels. 


———_ 


Geographical Position. Population. 








Kuram valley. (See Vote under XXI.) 30,C00 


Kuram valley, mostly about River Ariab and from 
the Shutar Gardan to the Paiwar Pass, 

| MNote.—XX. and XXI, are not regarded as true 

Patbans, being traditionally sprung of two 

Mughal brothers, Tor and Jaji. Edwardes 

says they are Khatar Hindkis from Rawalpindi. 





«In the hills between Miranzae and Kiiram. 


| 

| Dawari valley, 32° 57’-33° 7’ N. lat. 

} 

Upper Khost valley, adjoining Kiram and 
Zurmat. 

| 

| On Lajhi river, Kuram valley, and parts of 

Zurmat; are supposed to be of Mughal 

descent. 


East of Zurmat, E. side of Suleiman Mts. 


} 
| 
| 
| The hills opposite extreme S. part Dera Ishmail 
| district. Are disowned by the Afghans, though 
| apparently of Lohani (Povindah) stock. 


| 

| The hills west of Dera Ishmail Khan, Are said 
to be of Kakar origin, though now distinct ; 
Troglodytes. 


Between the Bij spur of the Suleiman Mts, and 


the Bozdar Biloches. _- 


| 
| 
| 


3,521,000 








Of the main sections in this table, Nos. I. to XII. inclu- 
sive are recognised as true Afghans, and of these, Nos. I. 
and III. (Duranis and Ghilzaes) are by far the most impor- 
tant and influential. Since the time of Nadir Shah, the 
Durdanis have been the ruling tribe, the Popalzae division 
till 1818, the Barakzae from that year to the present 
time. They were formerly called the Abdali or Avdali, 
a name which has been traced to the Ephthalites and 
Abdela of the Byzantine writers of the sixth century. But 
it was changed to Durdni from the title of Durri-Duran, 
** Pearl of the Age,” assumed by the Sardar Ahmad Khan, 
of the Saddozae branch of the Popalzaes, when he 
usurped the supreme power at Kandahar on the death 
of Nadir Shah in 1747. The seat of government was 
removed from Kandahar to KA4bul by his successor, 
Taimin Shah (ob. 1793), and this dynasty became ex- 
tinct in 1818, when it was succeeded by the Barokzaes 
in Kabul, though various descendants of Ahmad Khan 
continued and still continue to assert their claims to the 
sovereignty in Herat. 

Although mentioned in the national genealogies, the 
right of the Ghilzaes to be considered as Pukhtins at all, 
much less genuine Afghans, has been questioned. There 
certainly seems to be a flaw in their escutcheon, and they 
themselves, who always call themselves GAz/j7, and not 

1 I have not yet succeeded in obtaining the subdivisions of this section, 
and will feel obliged ifany reader of NATURE will kindly communicate them, 

with any other omissions or rectifications that may occur to him. 








Ghil-zae, claim Tiirki descent. The national tradition is 
that they entered the country in the tenth century under 
a certain Sabaktakin, of the Kilich Tirki tribe “ anciently 
situated on the upper course of the Yaxartes”? (Syr 
Darya). But, however this be, they are now entirely assimi- 
lated in habits, dress, religion, and speech, to the other 
Afghan tribes, with the exception of a few who are still 
nomads, 

None of the other sections call for special remark 
except the Povindahs, who are at once agriculturists, 
traders, and warriors, their armed caravans yearly fighting 
their way through the intervening hostile tribes down to 
the markets of the Panjab and Sindh. The name is 
supposed to derive from the Persian Parwinda, a bale of 
goods, and: seems to be indifferently applied to the 
Lohanis, Waziris, Kakars, Ghilzaes, or any other tribe 
temporarily or permanently forming part of this singular 
“trades’ union.” By far the most important section are 
the Lohanis, the oldest and most numerous members of 
the association, and one of the most promising elements 
for the future pacific settlement and material prospects of 
the country. 

Physically the Afghans may be described as, on the 
whole, a fine race. Their features, though often coarse 
and ugly, are regular in the European sense of the term, 
with the occasional Jewish cast above remarked upon. 


? H. W. Bellew, “ Afghanistan and the Aghans,”’ 1879. 





= -@ owt ot oe. 3lUdElC lr 


os ate tt Oe) oe ee Oth & OF 8 oe om ot oe A Ue lt os ee 


Fan. 22, 1880] 


NATURE 


281 





Type, long, oval face, arched nose, head mesaticephalous, 
that is, intermediate between the round and the long, 
measured horizontally, with cranial index 79 ;1 fair com- 
plexion, thick beard, hair and eyes generally black, but 
light blue or grey eyes and brown hair common amongst 
the Rohillas,? as the Suleiman highlanders are often col- 
lectively called. 

The great bulk of the people are Sunnites, which is 
one of the causes of their profound aversion to the 
Persians, who are mainly of the Shiah sect. Yet the 
nobles and upper classes, especially amongst the DurAnis, 
usually converse and always correspond in Persian. The 
consequence is that the Pukhtu, or national language, has 
remained a somewhat rude idiom, seldom employed in 
literature, and in refined society regarded as little better 
than a provincial patois. Its importance philvlogically is 
considerable, for though usually grouped with the Iranian 
branch of the Aryan family, Dr. Ernest Trumpp (Gram- 
mar, 1873), gives it a more independent position as inter- 
mediate between the Iranic and Indic, while Prof. Haug, 
of Munich, now regards it as a separate member of the 
family. It is very harsh and spoken with considerable 
dialectic variety everywhere in Afghanistan proper except 
the Hazarajat, and also in the Peshawar district of British 
India. The most marked dialects seem to be the Kanda- 
hari, Dir, Tirhai, Peshawari, Khaibari, Tarni, Vaziri, and 
Ushtarani. The Pashae and LaghmAni, sometimes in- 
cluded in the list, are not Pukhtu at all, or even Iranian, 
but distinctly Sanskritic, closely allied to the Siah Posh 
and Kohistani. A. H. KEANE 





THE METEOROLOGY OF SOUTH 
AUSTRALIA * 


M® CHARLES TODD sends us a well-written and 

eminently practical paper on the rainfall of 
Adelaide during 1878, illustrated with a map showing the 
positions of the 115 stations for the observation of the 
rainfall of that part of Australia and their rainfall for the 
year. Along with the monthly rainfall for 1878 there are 
printed the monthly means of forty-three of the stations 
at which the rainfall has been recorded for at least eight 
years. Since these stations extend right across the con- 
tinent from Palmerston in the north to Cape Northum- 
berland in the south, we are now, through this boldly 
designed system of observation, obtaining just notions of 
the agricultural and pastoral capabilities of the colony, in 
so far as these depend on that prime factor of climate, the 
rainfall, 

The rainfall of South Australia depends, on the one 
hand, on the tropical rains, which extend from the north 
coast inland, and prevail from November to April ; and 
on the other hand on the winter rains, which extend from 
the south coast northwards into the interior, and prevail 
for the seven months ending with October. 

The tropical rains extend in a greater or less degree 
across the interior, as far as lat. 26 S., falling off very 
considerably, however, south of Daly Waters, in lat. 16° 
15’. The breadth over which these rains spread south- 
wards and their copiousness depend altogether on the 
strength and southerly dip of the north-west monsoon, 
and consequently in the years when this monsoon blows 
over Australia with diminished force, a large tract of 
territory becomes nothing but an arid waste. 

A different state of things, however, prevails along the 
north coast and for a few hundred miles inland. There 
the summer rains fail not. At Palmerston, for example, 
the average of the past nine years gives a monthly fall 


y | gee Oe nae Cone.” 
rom = ersian = i i i 
Northern Fae * mountain, whence also Rohilcund, in 
3 “* Meteorological Observations made at Adelaide Observat: durii 
1876~ ~ Pane ewe ay oy Todd, CMG. FRAS 
oO uu ustralia durin 8” (with Char: 
Heh aa Oe One tee 





for each of the four months, from December to March, 
of 12°38 inches; in April, October, and November, the 
monthly mean is 3°68 inches; in May and September it 
is small, and in June, July, and August no rain falls. 
Here, then, is a large region, doubtless with a great 
future before it as regards the supply of the markets of 
the world with fruits and other tropical produce, such as 
have long been shipped from the rich plains of India and 
Ceylon. 

The winter rains occasionally extend well up into the 
interior, sometimes passing the centre of the continent; 
but generally they thin off about 1oo miles north of 
Spencer’s Gulf, and are heavy north of this gulf only 
along the Flinder’s range of mountains. The area of 
minimum rainfall of the continent extends from the Great 
Australian Bight to the northern extremity of the Flinder’s 
Range, over the plains to the east of this range up to 
latitude 25°, and spreads either way to within perhaps a 
few hundred miles of the east and west coasts. 

The agricultural districts of South Australia are marked 
off by the method of distribution of these winter rains ; and. 
roughly speaking, they lie for some distance northwards 
along and in the immediate vicinity of the Flinder’s 
Range, and thence southwards along the coast to Cape 
Northumberland. This broadish strip of territory con- 
stitutes, then, the granary of the colony ; and looking at 
Mr. Todd’s rain returns in connection with the broad 
physical features of the region, it is likely always to 
remain so, 

The close connection between the average quantity 
of wheat reaped per acre and the rainfall is shown in a 
table, giving for each year beginning with 1861 the yield 
per acre and the monthly rainfalls deduced from the 
observations of rain made over the agricultural districts 
during these eighteen years. In 1878 the rainfall over the 
agricultural districts was nearly 3 inches under the average, 
and the yield of wheat was only 7 bushels 9 lbs., or nearly 
three bushels under the average. Still more instructive 
would the comparison be if, instead of lumping the districts 
together, their average rainfalland average yield of wheat 
were presented in a separate form. 

The Meteorological Observations made at Adelaide 
Observatory, published monthly, show also the rainfall at 
all the rain stations with remarks, the appearance of 
which cannot but be watched with the liveliest interest by 
the Colonists. Thus in January, 1876, it is noted that 
the monsoon scarcely reached the MacDonnell Ranges, 
south of which, and as far as the east coast, drought 
prevailed; and in the following month the information is 
given that although 10 inches of rain fell at Port Darwin, 
the monsoon rains were comparatively light and barely 
reached the centre of the continent. 

The observations at the Adelaide Observatory are 
made, printed, and discussed with extremely satisfactory 
fulness for an observatory not furnished with continu- 
ously recording instruments. Of special value are the 
comparisons made of each month’s observations with the 
means of these months from past observations. The 
sorting of the wind observations into the directions for 
each hour of observation, viz., 6 and 9 A.M., noon, 3, 6, 
and 9 P.M., give most interesting results. These show for 
the summer months a shifting of the wind from a south- 
easterly direction in the morning to a south-westerly 
direction in the afternoon, a result doubtless due to the 
situation of Adelaide with reference to the heated inte- 
rior of the continent, as that heating varies during the 
twenty-four hours, 

The weak point of this system of meteorological obser- 
vation is the total absence of barometrical and thermo- 
metrical observations at all the stations except Adelaide. 
Such observations were made at some half dozen stations 
during 1861-64, but since then we miss them from the 
reports. It would not be possible to exaggerate the 
importance, not only to the colonists themselves, but to 





282 


NATURE 


| Fan. 22, 1880 





the whole body of meteorologists over the globe, of the 
establishment of such a system of weather observation 
across this continent ; and, moreover, the establishment 
of an efficient system of stations with their necessary 
equipment of instruments and observers, could not be in 
better hands than his whose resolute will and organising 
genius girdled Australia with the telegraph. 





ALG} 


PRO: J. G. AGARDH has taken advantage of the 

leisure afforded by his retirement from the Chair of 
Botany which he has filled so successfully for many years 
at the Lund University, to compose another work on 
algology. This very interesting volume, which embodies 
the results of observations made by the Professor 
during a long course of years, on the Morphology of 
the Floridez, has just appeared in the 7vansactions of 
-the Scientific Academy of Stockholm. It is written in the 
Swedish language, and is illustrated by thirty-three 
coloured plates of rare and little-known alge, and of 
microscopic details of many others, beautifully executed 
by Swedish artists. It treats the subject in an exhaustive 
manner, as will be seen from a specification of the 
contents. The work is divided into three parts, each 
part being copiously illustrated by reference to the plates, 
and to descriptions of different genera and species. 

Part I. treats of the general aspect and outer part of 
the Floridew—their development and growth; of the 
root and its different forms; of the stem, branches, and 
leaves. 

Part II., treating of the structure of the Floridez, 
describes the nature of the cell-membrane and of the 
cuticle; the contents of the cell under different con- 
ditions of development; the various layers or strata of 
which the thallus is composed ; the connection between 
the different cells, and the manner in which this connec- 
tion is effected; the various ways in which the cells are 
formed ; their different positions, and the manner in which 
they are grouped and united with the several strata. 

Part III. describes the reproductive organs, namely, the 
antheridia, the sphzerospores, and the capsular fruit and 
cystocarp, and concludes with remarks on the so-called 
“double fructification.” This third part will doubtless 
attract the attention of algologists who may be desirous of 
knowing whether the views of the Professor, in regard to 
the fertilisation of the fruit in the manner recorded by 
MM. Bornet and Thuret, have undergone any change 
since the publication of the “ Epicrisis ” in 1876. It will be. 
seen from the present work, that although Dr. Agardh 
has made multitudes of microscopic observations on 
British and exotic algz, at all periods of growth, and 
especially of the species which formed the subject of 
Bornet and Thuret’s experiments, he has not materially 
changed his opinion. He says that the observations 
hitherto recorded are too few in number to determine the 
question, and that, as yet, he has seen nothing confirmatory 
of the views of the French algologists. For his reasons 
and remarks we must refer the reader to the work itself. 
It is to be regretted that Dr. Dodel-Port’s very interesting 
observations on the fecundation of the Floridee by 
Infusoria, of which an ‘abstract was given in NATURE, 
vol. xx. p. 463, were not published before the completion 
of Prof. Agardh’s work. 

Among the verbal descriptions and illustrations are 
many which are especially deserving of the attention of 
British algologists. Among them will be found micro- 
scopic representations of the fruit, hitherto imperfectly 
described and figured, of many British alge. The cysto- 
carpic fruit of Cal/ithamnion cruciatum is now, it is be- 
lieved, figured for the first time. Among the whole figures 


t ““ Florideernes Morphologi,” af J. G. Agardh. Kongl. Svenska 
Vetenskaps Akademiens Handlingar, Bandet 15, No. 6 (1879). 
“De Algis Nove Zelandi# marinis.”” In supplementum “ Florx 


Hookerianz,” scripsit J. G. Agardh. Lunds Un‘v., Arsskrift. Tom xiv. 








of algz is one of a species which, although found on ou‘ 
southern shores, is almost unknown to collectors. Thi° 
species is Nitophyllum litteratum [Plate xxvii. Figs. 1-4) 
which may—but very rarely—be seen in collections under 
the name of VV. Aizi/ia. From this last-mentioned species 
it differs in form, being more lobed, and also in the fructi- 
fication. The sphzrospores, instead of being scattered 
over the disc as in WV. Hillia, are located between the 
numerous veins which mark the lower part of the frond. 
Minor differences are shown in the microscopic details. 
The capsular fruit of this species does not appear to be 
yet known. It therefore adds another instance to the 
long list of Florideze which hitherto have been found with 
sphzerosporic fruit only. 

There is some diversity of opinion as to the place ina 
general system of classification of certain algz of a red 
or purple colour, namely, Porphyra, Bangia, and Ba- 
trachospermum. By some of the later algologists they 
have been placed among the Floridez, but Prof. Agardh 
is of opinion that they do not belong to the red sea- 
weeds. 

There is another group of algz, which really belongs to 
the Floridez, whose position in the system still appears 
to be uncertain. We allude to the family, Corad/inee. 
We remember to have noticed that it is not included in 
the classification of the Floridez in the Epicrisis. We 
are, therefore, the more disappointed that there is no 
notice of this interesting group in the present work. Dr. 
Agardh’s observations with regard to it would be most 
welcome. Had the present very valuable work been 
written either in Latin or English, it would undoubtedly 
have been more serviceable ; as it is, however, algologists 
who do not understand Swedish may learn a great deal 
from the carefully-executed plates. Should the work be 
republished, it would be desirable to add a table of con- 
tents and an index. 

The “ List of New Zealand Algz’’ is a useful supple- 
ment to the “‘Flora Nove-Zelandize” of Hooker and 
Harvey. It consists chiefly of species which have been 
brought home by Dr. Berggren. The names of Hooker 
and Harvey have been generally adopted; but all the 
species described have been re-examined by Prof. Agardb, 
and many of them re-named in consequence of such re- 
examination. The new species and varieties are about 
sixty in number. Descriptions are given of new species, 
and copious notes on such of the already known species 
as require this addition are appended. M. P. M. 





GAS AND ELECTRICITY IN PARIS 
INCE the Jablochkoff light was established for the 
first time in the Avenue de I’ Opéra, it may be said 
that there has been in Paris a regular competition be- 
tween gas and electricity. The “‘ Compagnie Parisienne 
d’ Eclairage et de Chauffage’’ by gas is certainly one oi 
the largest in existence, as it possesses every gas-work in 
Paris, and almost every one in the vicinity. A system ol 
subterranean pipes and valves connects all these estab- 
lishments, so that gas generated in Courcelles can be sent 
to any part of the city and suburbs if required. All these 
different works were conducted as separate establish- 
ments before the fusion which took place in 1854, under 
the auspices of the then existing Imperial Government. 
Two of these establishments are worthy of note—La 
Villette, as being the largest, the site of experimental and 
chemical work, and Vaugirard, where the retorts are 
warmed by the Siemens’ heat-generating process. f 
Each of the twenty arrondissements of Paris has its 
special gas office. The Company also sells gas-engines, 
and makes great efforts to develop the use of gas as fuel 
for warming and cooking in private houses and shops. 
The price of gas is dearer in Paris than in any other 
capital of Europe, and the arrangements are difficult to 
understand without an explanation of the French munici- 
pal institutions. 











Fan, 22, 1880] 


NATURE 





283 





The cry for more light having been raised in 
consequence of the experiments conducted with elec- 
tricity, a new gas burner has been invented by the 
Compagnie Parisienne, and placed experimentally in 
several large public thoroughfares, principally the Rue du 
4 Septembre, the Place de la République, tormerly place du 
Chateau d’Eau, and a pavilion in the Halles Centrales. 
The burners used in the Rue du 4 Septembre are the 
largest, and all the new burners have been constructed on 
the same principle. The ordinary wing burners consume 
about 120 litres of gas each hour. In these improved 
lanterns six burners, representing an hourly consumption 
of 1,400 litres, have been placed at the six summits of a 
hexagon. In the centre is a hole for facilitating the 
introduction of air and better consumption. The effect is 
really highly satisfactory, and the luminous effect is far 
greater than in proportion to the gas consumed. A 
large number of coffee-houses, theatres, and first-class 
shops have adopted the burners for exterior use. It is 
impossible to use them within any building except 
markets, owing to the immense quantity of heat radiated, 
which would be a nuisance, at least in summer time. A 
number of these improved gas lamps have been placed in 
the Lyons railway station (passenger department), and 
will be, within a few days, used for competitive experi- 
ments with the Lontin electric light. 

Besides the hole for admission of air, a gas-pipe is 
placed in the central part of the lamp. The aperture has 
been disposed so that a small jet is always burning, and 
thus for lighting the Jamp it is sufficient to open the valve 
of the gas pipe, and the six peripheral burners are lighted 
at once. After midnight the jets are extinguished and 
the central one opened, burning with a consumption of 
120 litres per hour, or like an ordinary old gas-burner. 
The supplementary gas consumed by the city is paid for at 
a very cheap rate, about 1s. 6d. per thousand cubic feet. It 
must be said, moreover, that the Chambre Syndicale des 
Tissus and other commercial institutions have organised 
an agitation to oblige the Municipal Corporation to 
diminish the price of the gas. The Commission of the 
Municipal Council is at present deliberating upon that 
important question. A large factory, the Say Sugar 
Refinery, close to the Orleans Railway Station, built a 
private gas-work for its own use. They consume yearly 
about 6,000,000 cubic feet, and will turn their own gas- 
makers. 

In electrical lighting the division principle is repre- 
sented in Paris by the celebrated Jablochkoff candle, and 
a diversity of opinions have been expressed on the subject. 
The apparatus in itself requires no description, but it is 





necessary to explain the results which have been obtained. | 
The Jablochkoff light, placed in an opal globe is consi- | 


dered as perfectly suited to large shops and large public 
thoroughfares, although the diminution of light by the 
interposition of the globe may be valued at 45 per cent. 
The price of effective light is enlarged in the same pro- 
portion. This isthe reason why many persons suppose that 
from an economical point of view it will never do except 
in large open places, as the Place de la Bastille, where 
semi-transparent globes are used without fear of any com- 
plaints from shopmen or street passengers. But even for 
illuminating these large places, it is supposed by many 


competent persons that other electric lights would be | 


more successful, and at all events more economical. 
The only place where the Jablochkoff candles can 
be considered as unrivalled are large establishments 
like the Grands Magasins du Louvre, the Buttes 
Chaumont and the Ville de France, where the effect 
obtained is alone considered without much regard to the 
expense. The illumination of the Palais de l’Industrie 
during the evening sittings of the Exhibition of Fine Arts, 
was a success last summer, It was not attempted a second 
time during the Exhibition of Sciences Applied to 
Industry, owing to several circumstances, having nothing 





to do with the value of the system. At the Hippodrome 
the illumination is effected by a combination of gas lights 
and Jablochkoff candles, and ordinary regulators with 
luminous points carefully concealed. The general effect 
is quite satisfactory, but the expense in motive power is 
considerable. 

Jablochkoff candles are used in the illumination of 
large works carried on at present on the Seine for re- 
pairing the Pont des Invalides. These works have been 
interrupted for the last month owing to the frosty 
weather, but the Jablochkoff light has worked admirably. 
The use of the Jablochkoff candles is progressing im- 
mensely in private establishments, although the Municipal 
Council will in all probability discontinue the electric 
lighting of the Avenue de l’Opéra, the Place de la 
Bastille, &c., from February 1, and keep it burning 
only on the Place de Opéra. This impending resolution 
is attributed to the prevalence of the gas interest. 

In the first months of the Jablochkoff trial, many com- 
plaints were made against the irregularities of the light ; 
now extinctions are almost unknown, and the red colour 
of the electric flame less frequent. 

Extensive preparations have been made in the green 
room of the opera for a comparison between Jablochkoff 
and Werdermann candles, and will be completed in a few 
weeks. It is argued by Werdermann’s opponents that his 
light is merely incandescent light, and that the loss of 
illuminating power is far greater than with the Jablochkoff 
system. M. Garnier, the architect, being intrusted with the 
task of reporting on the matter, it would be unbecoming to 
give an opinion before his verdict is published. M. Reynier 
has another incandescent light offering some analogy 
with Werdermann’s, but the contact being more intimate, 
the loss in power is larger, and the public exhibition of it 
has been considered a failure. It is regarded as merely 
an apparatus for lecturers wishing to show their audience 
an electric light with few elements. The lamp is cheap, 
and its working quite regular. 

It should not be forgotten that even naked Jablochkoff 
lights lose a part fof their illuminating power. A quan- 
tity of electricity, which may be valued at 30 per cent., 
passes through the insulating caolin or plaster. Conse- 
quently it must not be wondered at, if some inventors 
tried to dispense with insulating lamina. 

M. Denayrouze, the former lessee of the Jablochkoff 
candle, has purchased the Jamin candle, in which the 


| electric flame is directed by the attractive power of 


magnetism or electricity. Private experiments have been 
made, and they are preparing for an exhibition in one of 
the suburbs of Paris. M. Jamin having to lecture at the 
Sorbonne on January 17 it is probable that the large hall 
will be illuminated by his own light on this occasion. 
This light company has purchased a patent for gas 
engines, and will try to use the gas under the furnace as 
fuel, dispensing with it for illumination. They are said 
to contemplate a public issue of shares for a large capital. 

It is known that the principal difficulties in the con- 
struction of regulators, has always been the absolute 
fixity of the luminous point in space. It has led M. 
Serrin tothe invention of his excellent regulator, But the 
use of the Jablochkoff light proved that inventors had 
gone too far in the way of complication, at least for 
street illumination, and where no dioptric or catoptric 
arrangement is contemplated. M. Suisse was the first to 
start a lamp which may be regarded as a simplification of 
Serrin’s original, and is working very well. The carbon 
is placed upwards, and descends -in proportion as the 
negative is consumed. In order to diminish that con- 
sumption the diameter of the negative carbon has been 
enlarged. Le BS 

A number of regulators have been tried in competition 


t It shows that a Jablechkoff candle placed in an opaque globe is dimin- 
ished (1) 0°70 by the loss of the caolin, and (2) o’50 by the opacity of the 
globe, so that it gives only 0°35 of the original illuminating power. 





284 


ATURE 


[ Fan, 22, 1880 





or will be, but Suisse’s is now the only one which works 
regularly at the Lyons railway terminus, in conjunction with 
a few of Lontin’s regulators and with Lontin’s generator. 
The results of the illumination are quite satisfactory, 
eighteen lamps being fed at an expense of 36 kilogrammes 
of charcoal per hour during fifteen hours every day, and 
with an expense of 9 francs per hour, including three 
francs of royalty for the Lontin Company. When this 
extensive space was illuminated by gas, the expense at 
19 centimes per cubic metre was 6 francs per hour, 
and would have been nine francs if the gas were charged 
30 centimes, or the full price. The economy for the 
Company results from the immense augmentation of the 
light distributed. They were enabled to diminish by 70 

r cent. the number of hands engaged in night work, 
and the risks from fire are reduced to nothing. Lontin’s 
system will be tried within a few days, in competition 
with improved gas, on the platform of the passengers 
department. 

At the exhibition of the Palais de l’Industrie, Lontin’s 
machine is working regularly every day from two to 
the closing hour, which varied according to the hour of 
sunset. No accident has been recorded. Siemens’s 
machine has been very seldom at work, owing to several 
circumstances which prevented the public from making 
a direct comparison. The engineer of M. Siemens’s fac- 
tory having been selected as one of the jurymen, Siemens’s 
machine was 7fso facto out of competition ; consequently 
we will not risk giving any definite opinion at present, 
confining ourselves to known facts. We visited Siemens’s 
light at the works established by the universal firm at 
Passy, and we were very much satisfied with the effect 
which we witnessed. The illuminating power and regu- 
larity were out of question. 

All the work of the Jablochkoff candle is done with 
Gramme machines, which have been fitted with a current 
inverter. 

Lontin, Suisse, and other regulators are worked with 
continuous currents, which is considered as more advan- 
tageous. 

Three different magneto-electric generators are before 
the public: Gramme, Lontin, and Siemens, based on 
similar principles, having a strong similarity in many 
respects, each of them claiming priority. We cannot 
presume to give a definite opinion on their special value, 
or on the value of their respective claims. The question 
can only be settled by the city or the Government 
deciding for the illumination of some part of the city or 
of some large public buildings. 

We can state, at all events, that the Meritens Company, 
has started new machines, which we witnessed working 
with regularity at the Continental Hotel on the occasion 
of a great ball; that the Alliance machine, although 
excellent for lighthouses, has proved too heavy, too ex- 

nsive, and too cumbrous for ordinary purposes. The 

ontin machine is rotated at a rate of 200 or 250 turns 
per minute, and its rival from 700 to 800, which is a 
decided advantage in its favour. 

It is not our province to adjust the claims relating to 
the manner of exciting almost any number of currents 
with a single generator and an electro-magnetic divider. 
But all the visitors to the Palais de l’ Industrie have been 
astonished by the regularity of the Lontin light and its 
facility of combining the several arcs. 

The other day the Ouest Railway Company established 
in the terminus of La Rue Saint Lazare three rival lights : 
Lontin, Parisian Company’s improved lights, and Jab- 
lochkoff candles. 

We decline to give a definite opinion of the respective 
merits of the Lontin and Jablochkoff systems before the 
moment when the numerous measures officially taken 
with a new photometer and the expenses in coals, electric 
carbon, and oil will be made public ; but we can say that 

s-light seems to be one-third dearer, and one-hal? only 
in general intensity. 





Some of the great expectations raised when the Ja- 
blochkoff light was first exhibited have proved groundless, 
The shares of the gas companies have recovered from 
their depression, and reached at least their former value. 
But it cannot be said gas has conquered electricity, as 
electric lighting, with all its variety of origin and regula- 
tion, is gaining ground daily. Siemens’s agents are at 
present fitting a large factory at Meaux with their regu- 
lators and generators. The works of installation of the 
Senate and Chamber of Deputies would have been im- 
possible without the help of the electric light. A new 
influential daily paper, Gi/ Blas, has opened on the 
Boulevard de )’Opéra an ‘Halle aux Nouvelles,”’ with 
no less than eight Jablochkoff candles. There is no 
part of Paris where electric lighting has not been exhibited, 
and its appearance is no longer a novelty, which is an all- 
important thing for its propagation. 

In the meantime there are other inventors trying to 
generate electricity by new means. M. Beaudet has 
started a bichromate battery which he calls uxpolarisad/e, 
perhaps without any real ground, but which, at all events, 
keeps in tolerable regulation for many days. M. Clamond 
has continued to produce a real electric light out of a 
series of thermal elements, which was considered as a 
mere impossibility a few months ago. We cannot say if 
the scheme of lighting by electricity out of a stove which 
warms an establishment, or a furnace which creates 
steam, is a Utopia, but we witnessed during some hours a 
light generated by the Clamond process, and a large work- 
shop uses no other lighting process during the present 
winter. 

The Municipal Council of Paris should open a public 
competition for lighting a large place or building, and 
invite all inventors of regulators and magneto-electric 
machines to place their apparatus in the hands of a com- 
petent commission, otherwise the question of electric 
lighting will remain in the dark for years, as it will be 
impossible for private individuals to decide which is the 
cheapest light produced and the best regulator. 

W. DE FONVIELLE 





NOTES 

WE regret to have to announce the death of Mr. George Wharton 
Simpson, the editor of the Photographic News, which took place 
at Catford Bridge on the 15th inst. He was well known to the 
large circle of amateur and professional {photographers as an 
able chemist, a lucid writer, and a careful experimenter. As one 
of the very earliest followers of photography, he was fully 
acquainted with all the many phases through which that technical 
science has passed, and we believe that very rarely, if ever, did 
he err in a matter of phctographic history or technology. There 
existed between the readers of his journal and himself a feeling 
of almost personal friendship, as no question was too trivial to be 
answered in his notices to correspondents, and the answer given 
was always of a kindly and helpful nature. To Mr. Simpson we 
owe, amongst other things, the perfecting of the collodio-chloride 
process, a process which for delicacy and permanency is up till 
now unrivalled. Mr. Simpson was also an occasional contri- 
butor to various daily and other journals, and some of these 
articles we hope may be reprinted, since they are really succinct 
histories of progress in the art-science with which he was so 
greatly bound up. He will not easily be replaced in his editorial 
position, since there are few, if any, who have lived through the 
stirring times which have made photography what it is, and have 
followed it with the attention which he bestowed upon it. The 
large gathering of literary men and photographers at Abney 
Park Cemetery on Tuesday last evinced the high esteem in which 
he was held. 

Ir is rumoured that Dr. William Ogle, Fellow of Corpus 
Christi, Oxford, and Examiner in Natural Science in the 





Fan. 22, 1880] 


NATURE 


285 





University, has been appointed to succeed Dr, Farr in the Regis- 
trar-General’s Office. 


Sir JosePH Fayrer, K.C.S.I., has been appointed Examiner 
for the Medical Service of the Army in Anatomy and Physio- 
logy, vice George Busk, F.R.C.S., who has resigned the 
appointment, 


THE first meeting of the Society of Telegraph Engineers will 
take place on Wednesday, the 28th inst., when Mr. Preece, the 
new president, will deliver his introductory address. 





M. Dumas, who is the Chancellor of the French Academy, 
pronounced the speech in answer to M. Taine, the new member. | 
Everybody was struck by the spirited delivery and eloquence of 
the venerable perpetual secretary of the Academy of Sciences. 
The house was so full that even academicians were unable to find | 
room on their benches. 


Mr. CROOKEs has been exhibiting his wonderful experiments | 
on radiant matter in Paris at the Ecole de Médecine, on Thursday, 
January 8, and on Saturday, the 11th; at the Observatory on 
Thursday, the 15th; and at the Société de Physique on Friday, 
the 16th. On all these occasions Mr. Crookes met with great | 
success. M, Salle, a well-known physicist, spoke in the name | 
of Mr. Crookes, who superintended the experiments. M. 
Gambetta and the Ministers of Public Works and of War were 
present at the Observatory, as well as the most influential 
members of the Institute. 


THE Zimes Philadelphia Correspondent telegraphs on Sunday 
that the Edison electric lights in Menlo Park were still burning to | 
the extent of about eighty lamps. Mr. Edison, finding that defective | 
vacuums have developed in a considerable percentage of the 
lamps, has for several days been experimenting to improve the 
mechanical construction of the glass globe containing the light 
so as to insure a permanent vacuum. Mr. Edison’s friends 
report that he is able to overcome the difficulty. Meanwhile, 
the manufacturing of additional lamps has .heen delayed, while 
no arrangements have yet been made practically to use the light 
in New York, 

THE correspondent of the Mew York Herald has interviewed 
M.Dumas, M. Niaudet Breguet, Mr. Crookes, and M. Fontaine, 
the president of the newly established Syndicat d’Electricité. 
The object of the interviews was to obtain the opinion of these 
gentlemen on the Edison light, and the results have been tele- 
graphed to America, We can state that they are not against the 
possibility of the success of Mr. Edison. 


WE notice an important communication which was made by 
Prof. Kessler at the annual meeting of the St. Petersburg Society 
of Naturalists on January 8, on the ‘‘ Law of Mutual Help,” as 
one of the chief agents in the development and progress of 
organisms. Prof. Kessler, although an able follower of Darwinism, 
thinks that the struggle for existence would be insufficient to 
explain the progress in organic life, if another law, that of 
sociability and of mutual help did not powerfully work for the 
improvement of the organisms and for strengthening the species. 
M. Severtsoff warmly supported this view, quoting several 
examples which prove that the unsociable birds are in a state of 
decay; so, for instance, although the system of robbing is 
ideally organised by the hawks, nevertheless the species is in a 
state of decay precisely because of its want of sociability. 


ON January 10 the Russian Physical and Chemical Society 
held at St. Petersburg its annual meeting. After the reports of 
the secretaries Prof, Mendeleeff gave an interesting address on 
the resistance of fluids ; he gave an historical sketch of the sub- 
ject, and, pointing out how little it has hitherto been investigated, 
and how important it is, he invited Russian physicists to give 
special attention to that part of hydrodynamics, Prof, N. 





| the body. 


Beketoff, from Kharkoff, read a paper on the dynamics of 
chemical reactions, and explained the electro-dynamical theory 
he proposes to explain them. Prof. Lentz made a communica. 


| tion on electrolysis, and M. Jablochkoff exhibited his new 


galvanic element. 


M. LE Bon, in rendering an account of the progress of his 
observations on the comparative mean weights of male and 
female skulls (Au//, of Paris Anthrop. Soc, t. v. fasc. 5) has 
explained the precautions which he had taken to avoid errors 
arising from considerations of the differences, bodily stature, age, 
race, and social or civilised status. After taking all these con- 
ditions into account, he finds a difference of 172 grammes in 
favour of the skulls of men over those of women. He asserts 
that while a newly-born girl has a heavier brain than a newly 
born boy—an advantage which she rapidly loses—the women of 
inferior races are relatively superior to those of highly civilised 
races, in other words, woman does not advance, and consequently, 
the differences between her and man are constantly augmenting. 
If M, le Bon’s assertions are to be accepted as facts, they would 
undoubtedly seem to point to the necessity of bringing the oppor- 
tunities of intellectual culture more closely within reach of women, 
but the learned doctor predicts that the abomination of desolation 
will fall on society if women be removed from the happy ignorance 
of their domestic hearths, Apart from his avowed preference 
for women with the cerebral capacities of savages, M. le Bon’s 


| memoir will be found of great use to the student of craniology, 


by helping him to determine the mathematical relations of 
different parts of the head, and their bearing on other parts of 
We are glad to learn that the great value of his work 
in elucidating various obscure questions of general anthropology, 
have secured for it the award of the Godard prize for 1879. 


AT Vienna a ‘‘ Verein fiir Héhlenkunde” has been formed» 
with the object of investigating caves. Everybody taking an 
interest in this subject may become a member. The subscription 
is only 5 florins per annum, Dr, Franz von Hauer is the 
president, and Prof, Ferdinand von Hochstetter the vice-pre- 
sident of the new Society. 


THE next German Anthropological Congress will be held at 
Berlin early in August next, and will be accompanied by an 
exhibition, illustrating prehistoric times in Germany. It will be 
closely followed by a Geological Congress to be held in the same 
city. 

A MONUMENT of the late eminent naturalist and horticulturist, 
Freiherr von Siebold, will shortly be erected in his native town 
of Wiirzburg. 


THE Japan papers record the fact that an enormous piece of 
coral was lately dredged up near Tosa, It is stated to have five 
branches, the stem being 15 inches in circumference and 5 feet 
in length. 


THE Section of the Society of Arts formed in 1874 for the 
discussion of subjects connected with practical chemistry and its 
applications to the arts and manufactures, has been this year 
enlarged in its scope that it may include applications of physics 
as well as chemistry. At the six meetings of the present year 
the following papers will be read. The meetings are on Thursday 
evenings at eight o’clock, and the dates have been selected so 
that they do not clash with those on which the meetings of the 
Chemical Society are held :—January 22, ‘* The Teaching of 
Technical Physics,” by John Perry, late Professor of Engineer- 
ing, Japan ; February 12, ‘Gas Furnaces and Kilns for Burning 
Pottery,” by Herbert Guthrie, C.E.; March 11, “The Noxious 
Gases Bill,” by Dr. S. K. Muspratt, F.C.S.; April 8, “On 
Recent Improvements in Benzine Colours,” by F, J. Friswell, 
F.C.S.; April 22, ‘On some Recent Advances in the Science 





286 


NATURE 


[ Fan, 22, 1880 





of Photography,” by Capt. Abney, F.R.S.; May 13, ‘On 
some Physical Applications of Light,” by Prof. W. G. Adams, 
F.R.S. 


THE Zhunderer gun experiments were continued at Woolwich 
last Friday, the object on that day being to test what is known 
as the “‘ wedging” theory—the supposition that the tilting or 
displacement of the wad had to do with the bursting of the 
original gun. The experiments on Friday tended clearly to dis- 
prove this theory. 


THE Public Works Department at Yedo have just published 
the Reports of Progress for 1878 and 1879 of the Geological 
Survey of Japan under Mr. B. S. Lyman. 


THE Indian papers state that experiments are about to be 
made in Cyprus to test the possibility of cultivating mango 
seeds, as well as the seeds of other Indian fruits and vegetables. 


EARTHQUAKES are reported (1) from Weisskirchen, where on 
December 22 at 5 A.M. a violent shock was felt ; (2) from St. 
Blasien, in the Black Forest, where a shock was noticed on the 
same day at 10 P.M. ; (3) from Idria (Carniola), where a subter- 
ranean explosion took place at 8.30 P.M., combined with a 
violent shaking of the ground and a cannon-like report. Several 
shocks were felt at Churwalden (Switzerland, canton of Chur) 
on January 7, between 2 and 4 A.M. ; the last shock was accom- 
panied with a noise like that of thunder, so that people were 
awoke and dogs howled. In the Domochleg and at Savagnino 
only two shocks were felt, at 3h. 45m. and at 4h. 3om. The 
shocks had the direction from north to south, 


At Freiburg, in Breisgau, the beautiful and rare pheno- 
menon of the fata morgana was observed at noon on December 
16. While the sun was shining the fine pyramid of the Cathedral 
tower showed itself reflected above, of course with the point 
downwards. The reflecting stratum of air was almost at the 
level of the summit of the tower, thus producing a most peculiar 
effect. 


WE are glad to see that the Epping Forest Field Club has 
been successfully formed, under the presidency of Mr. R. 
Meldola. From the tone which prevailed at the meeting of 
January 10, we should think the Club is likely to do good work. 
The original list of members is a pretty large one, and contains 
several well-known names. 


THE continuation of frosty weather has produced unprece- 
dented effects on the Lower Loire round Saumur. The bed 
of the river having an extent of about 1,000 yards, and the 
depth of water being very shallow, the Loire was entirely 
frozen and the flow of water towards the sea was almost entirely 
stopped. The consequence was that the level of the water was 
raised, and the walls protecting the low lands in danger of being 
submerged. It was necessary to employ dynamite to open a 
channel for the water. Unfortunately a part of the stream has 
found its way into the low lands. New ice is coming from the 
high lands, and the military have been ordered to work under 
the orders of civilian engineers. 


AN ascent of Mount Hekla was made last summer by a lady, 
Miss Th, Petursson, daughter of the Bishop of Reykjavik, for 
.the purpose of geological investigations. According to her 
observations the temperature at the bottom of the larger craters 
has of late risen considerably, while dense white columns of 
steam were rising from crevasses and holes which were hardly 
visible, The sulphurous odour of this steam was stronger than 
usual, The observations seem to indicate an approaching erup- 
tion of the volcano. 


AN interesting archxological discovery has been made near 
Lehmke (in the district of Oldenstadt) consisting of some 1,200 





medizeval metal plates, so-called dractee. Most of them bear 
the stamp of a lion in varying positions, others that of a figure 
with sword and standard, and a horizontal key below. - The 
objects in question are now in the possession of the ‘ Kreis- 
hauptmann ” of Oldenstadt. 


THE German Postmaster-General, Herr Stephan, and Dr. 
Siemens, have succeeded in constituting an electro-technical 
society, which has for its objects the furtherance and deve- 
lopment of the technical application of electricity, the 
progress of the knowledge of electricity by means of its technical 
appliances, and the establishment of a place of meeting for 
German technical electricians, whose scientific and commercial 
interests will, of course, be greatly benefited by such mutual 
intercourse, 


THE additions to the Zoological Society’s Gardens during the 
past week include a Rhesus Monkey (Afacacus erythreus) from 
India, presented by Mr. F. C, Grosvenor ; two Bankiva Jungle 
Fowls (Gallus bankiva), two Starred Tortoises (Zestudo stellata) 
from India, presented by Mr. W. Dunn, C.E., C.M.Z.S.; a 
Bar-tailed Godwit (Zimosa lapponica), a Grey Plover (Sguatarola 
helvetica), six Knots ( 7ringa canulus), thirteen Dualins (7ringa 
cinclus), European, presented by Mr. F. Cresswell; three 
Chinchillas (CAinchilla lanigera) from South America, a Grey 
Struthidea (Struthidea cinerea) from Australia, a Red-throated 
Amazon (Chrysotis collaria) from Jamaica, purchased; two 
Fulmar Petrels (Procellaria glacialis), North European, de- 
posited. 





OUR ASTRONOMICAL COLUMN 


THE ORION-TRAPEZIUM.—The following letter has been 
addressed. to us by Prof. Holden, of the Naval Observatory, 
Washington :— 

**In NATURE vol. xxi. p, 117, there is a note on a seventh 
star in the Orion-trapezium, which is 636 of G. P. Bond’s Cata- 
logue. It is there rated as mag. 13°3. Two other stars, 612 
and 618 of Bond’s catalogue are as near one of the larger stars as 
636 is, and if it is intended to extend the nomenclature of seventh 
star, eighth star, &c., to these stars (which seems inadvisable), 
they should be included. Their positions from @' Orionis are :— 

Mag. 4 u (1857'0) 4 4 (1857'0). 
612 13°5 — 16°4 + 24°6 
618 13°! — 104 + 24°6 
The magnitudes are too faint for Argelander’s scale extended, 
but serve to compare with that of 636 viz. 13°3. 

‘* As tests for large telescopes, quite a number of small stars 
discovered by Bond may be mentioned, whose positions are 
given in Annals of the Harvard College Observatory, vol. v. 
All of these really exist, as they have been repeatedly seen with 
the 26-inch refractor of this Observatory. They are Nos. 595 
(13°9m.), 601 (15°6), 608 (14°3), 621 (15°6), 625 (15°6), 631 
(14°3), 666 (13°9), 677 (14°8), 676 (13°1), 642 (15°6), 675 (15°2). 
The faintness of these stars (which are much better seen with a 
low power than with a high one) speaks well for the diligence of 
the late George Bond, whose search in this region was very 
thorough. Other small stars exist in the neighbourhood as 
follows :— 

**1, Rosse, No. 56, near G.P.B. No. 581. 

**2, A star, s.p., G.P.B. No. 724. 

**3. A double-star, n.f., G.P.B. No. 685. 

‘* (2 and 3 were discovered by Lassell.) ; 

‘*4. Three stars in or near the region bounded by the lines 
641 to 663, 663 to 652, 652 to 641. 

‘5. A star or mass of nebula which is not yet three years of 
age, has developed itself in the middle of the dark channel 
half way between 669 and 642. The star (?) itself is, roughly, 
equally distant from 669, 641, and 642. 

‘** There are no stars within the trapezium. 

“Cooper reports a star following G.P.B. 516 a few seconds. 
I cannot find it. ; 

‘* Any observations on these stars or on the celebrated variable 
654 (frequently observed here) will be gladly received by mé, 





¥an. 22, 1880] 


NATURE 


287 





and I shall be happy to have such for insertion in a paper now 
nearly ready on the Huyghenian region of this nebula.” 

For the convenience of such observers as may not have ready 
access to the ‘Annals of the Astronomical Observatory of 
Harvard College, vol. v.,” which contains G. P. Bond’s elabo- 
rate memoir on the nebula of Orion, the following differential 
positions of the stars mentioned by Prof. Holden, with reference 
to 6' Orionis, are extracted :— 


Diff. R.A. Diff. Decl. 


No. 516 ...—276°0 ...— 29°5 
581 ...— 76°L ...—159°1 
.- 46°9...- 15°0 
wi 36°O...- 310 
we 23°7...- 18°0 
.- 80...- 36°0 
w= 4 w- B 
ot 3 «.— 4 
oa 


Diff. R.A. Diff. Decl. 


No. 652...4 30°2...+171°6 

0s 3332... + 10°O 

55°5 ---+147'1 

59°7 -..—195°8 

63°3 ... + 100°0 

74°5 +» 93°4 

78°5 ...- 276 

78°6 ...—201°4 

wet ILQ... F1IU2 ws 97°T  — 950 

642...+ 13 «+ 48 724 ...+183°3 ...-—176°0 
It will be remarked that Prof. Holden states there are actually 
no stars within the trapezium. Mr. Burnham’s experience with 
the 184-inch refractor at Chicago is to the same effect. ; in the 
notes to his last catalogue of double stars, he writes : ‘‘ Several 
observers have seen, or believe they have seen, other minute 
stars in the trapezium, most of them using comparatively small 
apertures. While making the measures given above, and at other 
times, under very favourable conditions, the interior of the tra- 
pezium and the vicinity of the principal stars were carefully 
examined. There was not the slightest suspicion of any addi- 
tional stars. If the sixth star itself had been double, with a 
distance of 10, it could not have been overlooked. I have 
very little faith in the real existence of these suspected stars after 
the failure of this and other large refractors to show them.” And 
he considers it is wholly improbable that they should all be vari- 
able in such manner as to render them at all times invisible during 
the last few years. Telescopes were not s> perfect forty years 
since as they are now, and we might be perhaps justified in attri- 
buting to optical illusion the supposed existence of the three stars 
within the trapezium, recorded by De Vico in 1839, and the star, 
near the ‘‘ fifth,” detected by Struve, which Gruithui-en claimed 
to have discovered about the same time, and which he says 
Schwabe had also seen with a 6-feet Fraunhofer. But what are 
we to say to the observations of Dr, Huggins, as detailed in 
vol, xxvi. of the Monthly Notices of the Royal Astronomical 
Society? They appear to point to something more than optical 
illusion, and notwithstanding the negative testimony as to the 
actual existence of stars within the trapezium, to render it desir- 
able that a protracted examination of this region should be insti- 
tuted with telescopes of suitable capacity. One of Dr. Huggins’s 
stars is not far from the position of a star in De Vico’s diagram 
(see Memoria intorno a parecchie Osservazioni . . . in Collegio 
Romano, f Anno 1839, plate I., and Gruithuisen’s Astronomisches 

Fahriuch, 1841, p. 143. 


THE ToTAL SoLar EcLipsE oF JANUARY 11.—A Reuter’s 
telegram brings intelligence of the successful observation of the 
total phase in this eclipse on the Santa Lucia mountain, Cali- 
fornia, with the important addition that an intra-Mercurial planet 
has been again seen. In the longitude of this mountain the 
duration of totality upon the central line, employing the elements 
of the Nautical Almanac, would be only 38 seconds, with the 
sun at an altitude of 12°; if the semi-diameters adopted for 
eclipses in the American ephemeris are used, the duration would 
be even less—hardly 27 seconds. Under such circumstances it 
must have required very minute and skilful preparation and 
considerable smartness of execution to insure the results 
announced. 








GEOLOGICAL NOTES 


THE MSS. of Sartorius von Waltershausen, descriptive of 
Etna, have been placed, we understand, in the hands of Prof. 
von Lasaulx, of Breslau, with a view to publication. They will 
complete the colossal pile which the veteran geologist erected 
to the glory of his favourite mountain, 


ANOTHER distinguished and venerable vulcanologist, ‘Dr. 
Abich has gone to Vienna to prepare his petrographical descrip- 
tions of the Caucasian region, in which he has been so long at 
work, The facilities for the most delicate analyses of rocks and 





minerals at Vienna have likewise attracted thither M. Renard, of 
Brussels, who has been entrusted with the chemical and micro- 
scopic investigation of the abyssal deposits brought by the 
Challenger from its great ocean survey. M. Renard is at present 
in this country arranging with the Challenger Commission as to 
the prosecution and publication of his labours. His beautifully 
drawn plates which illustrate the more remarkable facts brought 
to light by the Challenger dredgings, are being exquisitely re- 
produced by chromolithography in Vienna, 

IN a recent number of the Bulletin of the United States 
Geological and Geographical Survey of the Territories (a 
publication still continued for a while, though the Survey itself 
has ceased to exist), Dr. F. V. Hayden describes the Two Ocean 
Pass which has for some years been known to separate the head 
waters of the Yellowstone from those of the Snake River. He 
confirms and extends previous accounts of this interesting locality, 
showing that it is a flat meadow-like depression cut by erosion 
on the watershed. During wet weather this marshy ground 
becomes a lake which drains both ways, one branch finding its 
way into the Pacific, and the other into the Atlantic, by one of 
the longest routes for running water on the surface of the planet. 


ProFr. MARSH continues his descriptions of the fossil treasures 
continually arriving to increase the already ample stores at Yale 
College. He remarks that while the Mosasauroid reptiles are 
so rare in Europe that the type-specimen described by Cuvier still 
remains the most perfect yet discovered here, and the only one 
from which important characters have been made out, in North 
America the group attsined a marvellous development, and was 
represented by several families with numerous genera and spe- 
cies, of which the relics of not less than 1,400 distinct individuals 
are contained in the museum at Yale. 


Dr. MICHEL Mourton of Brussels has in preparation a 
work on the geology of Belgium. It will form an octavo 
volume of at least 500 pages, containing full descriptions of the 
different geological formations, with unpublished plates of the 
microscopic structure of rocks, copious lists of fossils, and an 
account of the industrial resources of each formation, and will 
be followed by a complete bibliography of the geology, palzeon- 
tology, and lithology of Belgium, The re-issue of Dumont’s 
beautiful and most trustworthy geological map of Belgium natu- 
rally suggests the desirability of some general guide to the public 
in perusing the map or travelling through the country, for the 
admirable prodrome of M. Dewalque can hardly now be procured. 
Dr. Mourlon’s position as one of the Conservateurs of the Royal 
Museum of Natural History, and his experience as a field geolo- 
gist both before and since his connection with the Geological 
Survey of Belgium, give him exceptioral advantages for the 
preparation of such a work, which will no doubt be as duly 
appreciated by his fellow-countrymen as it will be welcomed by 
students of geology abroad. 





PHYSICAL NOTES 


OBSERVATIONS of phosphorescence phenomena in high vacua 
of the nature described by Crookes and Maskelyne have been 
lately made on a variety of substances by Herr Stiirtz of Bonn, 
in company with Herr Miiller (Wied. Ann. No. 11), The fol- 
lowing substances gave phosphorescence (those marked with an 
asterisk were made red hot before being brought into the tube ; 
in the ordinary state they showed little or no phosphorescence) :— 
Brucite,* magnesite,* phosphate of magnesia, pitch-blende, 
wolframite, cerusite, adularia, orthoclase,* -kaolin,* axinite,* 
silicate of zinc,* zinc-spar,* double spar, apatite, franklinite, 
azure spar, fergusonite,* apophyllite,* dolomite, ccelestine,* red 
spinelle, cobalt-glance, stannite, baryta, chromate of iron, lazu- 
lite, lepidolite, zinnwaldite, ankerite, greenockite, pectolith, 
borax, cinnabar, leucite, sanidin, and Java meteoric stone of 
1869. A few luminous points were observed in crystals of 
arsenical iron and antimonite. Pieces of a phosphorescent sub- 
stance made red hot are luminous with a different colour from 
that of pieces of the same not made red hot. In cerusite the 
phosphorescence is lost through heating. The authors give a list 
of substances which do not phosphoresce. 

A sysTEM of electrical storing, considered to be free from the 
disadvantages of other systems, is described by Professors 
Houston and Thomson in the Franklin Institute Yourmal for 
December, 1879. They use 2 saturated solution of zinc sulphate 
in a suitable vessel, having at the bottom a plate of copper, to 





288 


NATURE 


[ Fan. 22, 1880 





which is connected an insulated wire. At or near the top of the 
vessel, and immersed in the solution, is placed a second copper 
plate or one of hard carbon, or metal unchanged by contact with 
zinc sulphate solution and less positive than metallic zinc ; this is 
also connected with a wire. A current from a dynamo-electric 
machine is sent in the direction from the lower to the upper 
plate, the result being deposition of metallic zinc on the upper 
plate and the formation of a dense solution of copper sulphate 
overlying the under plate. The cell, after charging, constitutes 
a gravity cell, and continues a source of electrical current till re- 
conversion of all the copper sulphate into zinc sulphate, with 
deposition of copper on the lower plate and removal of zinc from 
the upper. The cells, in charging, may be arranged in multiple 
arc or in series, and differently from that in discharging, according 
to the object. The authors believe it possible to store and recover 
50 per cent. or more of the 50 or 60 per cent. which good 
dynamo-electric machines realise in external work of the power 
used in driving them. Thus 25 per cent. of the original power 
may be given out secondarily as electric current. Assuming that 
in the best steam engines 20 per cent. of the heat energy of the 
coal may be utilised, then about 5 per cent. of the heat energy, it 
is thought, may be recovered after storage as current ; but even 
with this small percentage the economy would be much superior 
to the use of zinc and other materials in the ordinary battery in 
production of current. 


IN a recent paper to the Vienna Academy, by Prof. Exner, on 
the theory of inconstant galvanic elements, proof is offered that 
there is no so-called galvanic polarisation in elements, but that 
the phenomena referred thereto are attributable to the oxygen 
dissolved in water. The electromotive force of an element with 
only one liquid appears accordingly as a constant which is in no 
way affected by any polarisation of the negative pole. It is 
further shown that the force of a Smee element is not altered 
when its platinum is replaced by some other metal, provided 
only this do not itself give rise to chemical processes. 





GEOGRAPHICAL NOTES 


Dr. Emit Houvs will read a paper before the Royal Geo- 
phical Society next Monday evening on his journey from the 
Diamond Fields through South Central Africa to the upper 
waters of the Zambesi. Dr. Holub, we understand, has for 
some time been exhibiting at Prague a small museum of zoo- 
logical and ethnographical curiosities collected during his various 
journeys in Southern Africa, which has attracted much attention, 
and he is coming to England to attend this meeting at the special 
invitation of the Council of the Geographical Society. 


THE Colonies and India reports the return of Mr. Alexander 
Mitchinson after some years spent in Africa. He appears to 
have arrived on the Gambia in 1876, and to have journeyed with 
a smal) number of followers into various parts of Africa. Fol- 
lowing the course of the Niger, he visited the waterfalls, and 
returning to the west coast, made excursions into the country in 
various directions. After a brief rest his travels were again 
resumed, and from the Gaboon country Mr. Mitchinson made 
his way into Angola, and from Benguela proceeded vid Bihé to 
Lake Ngami, returning to the coast at Walfisch Bay at the end 
of 1879. The notes which he made in the course of his travels, 
are said to contain much interesting matter. 


* IN the current number of the Zour du Monde M. Désiré 
Charnay, the well-known archzological explorer of Southern 
Mexico, Yucatan, and Madagascar, has commenced an account 
of what he saw during the six months he recently spent in Aus- 
tralia. His observations on the aborigines, their legends, cus- 
toms, and traditions will no doubt be interesting, and his story 
will certainly be well illustrated. M. Charnay, who returned to 
Europe not long since, had, previously to his visit to Australia, 
spent some time in the East Indian Archipelago, 


Dr. BENJAMIN BRADSHAW, who was met by Major Serpa 
Pinto, during his famous journey near the Zambesi, and who 
was also with the late Mr. Frank Oates when he died near the 
Tati settlement on his way from the Victoria Falls, arrived in 
Capetown a short time ago, presumably to make another trial of 
the ways of civilisation, Dr, Bradshaw has spent a long time 
in the Matabele country and other parts of the Zambesi basin, 
living the life of the natives and making zoological collections 
for his own amusement and benefit. During his wanderings he 
has acquired a considerable amount of information respecting 
the less-known parts of the Zambesi and some of its tributaries, 





ag we have reason to hope, may be made public before 
ong. 

A CORRESPONDENT in the Glasgow Herald advocates the 
formation of a geographical society in that great commercial 
centre, the second most populous city in the kingdom. We 
have on several occasions pointed out the advantages of the 
formation of such societies in our chief ports, by means of which 
much useful information might be tapped that otherwise would 
not see the light. No better field could be found for such a 
society than Glasgow. 


ProF. NORDENSKJGOLD and his staff evidently do not consider 
that their work was finished when they got outside Behring’s 
Strait in the Vega. During the brief stay of the ship at Galle 
they made excursions into the island to examine its mineralogy 
and natural history. Great preparations have been made for the 
reception of the Vega at Naples. The King of Sweden desires 
that the professor and the captain should visit Rome, Brussels, 
Paris, and London, and join the vessel again at Copenhagen, to 
be ultimately received at Stockholm. 


Dr. Otto FinscH left Honolulu on July 30 last,"on board 
the barque Hawaii, and arrived at Dshaloot, on the island of 
Bonham (the principal island of the Marshall group) on August 
21. He intended to investigate this island thoroughly, as it 
appears that this has never before been done in a scientific 
manner. From Bonham Dr. Finsch will proceed to the islands 
of the Radak group. 


News from Dr. Stecker, the well-known companion of Dr. 
Gerhard Rohlfs, stated that he was going to leave Benghasi at 
the beginning of the present month, in order to proceed to Bornu 
by way of Fezan. 

A FrRencH Company intends to cut a canal through the 
Isthmus of Corinth. Steps have already been taken to obtain 
the permission of the Greek Government. 

THE German residents of Sydney have founded a branch of 
the Berlin Central Union for Commercial Geography. 

Mr. 1M THURN, of the Georgetown Museum, whose labours 
in British Guiana have been referred to in NATURE, arrived in 
England last week. 





THE SIXTH CONGRESS OF RUSSIAN 
NATURALISTS 

THE Sixth Congress of Russian naturalists began at St. 

Petersburg on January 1, by a public meeting in the great 
hall of the University. The number of members present was 
very large—1,200—of whom 500. were from the provinces, and 
thirty-eight were ladies. Prof. Kessler was unanimously elected 
President, but the bad state of his health not allowing him to 
fulfil this function, he was made honorary president, Prof. 
Beketoff being elected as the active one. 

At the first public meeting, Prof. Wagner gave an interesting 
address on the ‘‘ Means of Solution of the complicated Problems 
of Natural Science,”’ and after a brilliant sketch of the methods 
of science, he drew the attention of naturalists to the necessity 
of the study of physiological chemistry, and especially of the 
problems connected with albuminous matters. 

Two — were then discussed :—On the scientific explo- 
ration of Bulgaria, and on the necessity of making complete 
botanical collections of Russian plants, 

The second public meeting of the Congress, held on January 7, 
was opened by an address by Prof. Timiriazeff, on the physio- 
logical significance of chlorophyll in the life of plants, on the 
absorption by it of solar rays, and on the limits of the produc- 
tivity of the soil. After this the president proposed that the 
several projects of scientific inquiries approved by the Congress 
be transmitted to a special committee, which would remain as @ 
permanent institution after the Congress, and see to the carrying 
out of these projects ; the proposal was unanimously accepted by 
the Congress, and will be accomplished, if the Ministry of Public 
Instruction does not oppose, as it has done hitherto, the creation 
of a permanent scientific association of all Russian naturalists. 
Prof. Mendeleef proposed the publication of a popular descrip- 
tion of Russian colonies, being a sketch of their climate, soil, 
flora, fauna, and economical conditions; the proposal was 
approved, Prof, Dobroslavine gave an address on the relations 
between natural sciences and hygiene. The latter has only one 


int in common with epee oan pathology—whilst any 
penguins in the department would be impossible if it were not for 





Fan. 22, 1880] 


NATURE 


289 





the collective work of those who labour in the wide field of 
natural «science, all most important advances in hygiene, being 
made by the researches of eminent specialists in natural science. 


Finally, Prof. Mendeleeff made the proposal to publish a new | 


scientific periodical, 

At the last public meeting of the Congress, Professors 
Sokhotsky and Kovalsky made a proposal to found a Russian 
Astronomical Society, and Prof, Tchebysheff proposed to solicit 
from the Government pecuniary help to the Moscow Mathe- 
matical Society ; both proposals were agreed to. 


tion of animals. Prof, Andreieff developed the idea as to the 
necessity of giving instruction in natural sciences in primary 
schools, and M. Gerd ;gave an address on the impulse which 
could be given to the study of nature in Russia, its flora, and 
fauna, by the teachers of the primary schools; he demonstrated 
by numerous facts that this help would be very effective, 


as a great number of teachers would be ver; glad to work on | 


that field ; therefore, he proposed to draw up good programmes 


for these studies, as well as simple manuals of the necessary | 
Both proposals were met with the warmest | 


elements of science. 
cheers of the numerous auditory, but we fear that they will meet, 
as have former proposals of that kind, with strong opposition from 
the actual Ministry of Public Instruction, After an address by 
Prof, Wagner, on the sociability of animals, the Congress closed 
its sittings ; the next Congress to be held at Odessa. 


following communications :—By Prof. Davidoff, on a new 
method for the exploration of functions, which method enables us 
to deduce various theorems from one general principle; by M. 
Preobrajensky, on the integration of Laplace’s equation by means 
of quaternions, the communication having given rise to very 
animated discussion ; and by M. Tchebysheff, on parallelograms, 
being a brilliant exposition of their importance in mechanics, 
together with a discussion of several points of theoretical import- 
ance. An interesting memoir was read by Prof. Bougaeff, on 
subtraction{in_the theory of numbers, which deals with several 
important philosophical points of mathematical investigation. 


Other communications were by MM. Markoff, Joukovsky, and Degree will again come on for discussion in congregation 


Vasilieff, on Bernoulli’s equation. 

In the Section of Physics and Meteorology we notice the fol- 
lowing communications :—By M. Ziloff, on the magnetisation of 
liquids ; by M. Collin, on the luminous properties of electrodes ; 
by Prof. Oettinger, on electricity ; by M. Pantionkhoff, on the 
meteorology of Bulgaria as compared with South-Western 
Russia; by Dr, Woeikof, on the various causes of perturbations 
in the diurnal changes of temperature; and by Baron Wrangel, 
on changes of level in the Black Sea, This level has continuous 
fluctuations ; it is always lower during the night, and reaches its 
maximum at mid-day in all sea-ports of the northern and the 
eastern coast; it is also at a minimum in October and a maxi- 
mum in May, the difference between these two levels being 18 
inches. The following communications of general interest were 
also made in the Section of Physics :—Dr. Woeikof exhibited a 
new map, showing the distribution of rainfall in all parts of the 
world; M. Borgmann made a communication on the influence 
of the inductive currents on the development of temperature 
during magnetisation; Prof, Lemstrém (Helsingfors) expounded 
his theory of terrestrial magnetism ; Prof. Tchebysheff read a 
memoir on centrifugal regulators, and exhibited two of his in- 
vention; and M. Tchikoleff, on electric lighting. 

_In the Section of Geology and Mineralogy we notice commu- 
nications by Prof. Lentz, on the level of the Amu-Darya; by 
Prof. Fr. Schmidt, on recent formations on the shores of the 
Gulf of Finland ; and by M, Armatelsky, on diluvial formations 
in the Government of Chernigov, 

_In the Sections of Botany and Zoology we notice the commu- 
nications by M. Tikhomiroff on the bacteria which cause disease 
of the bladder, and on the artificial production of these bac- 
teria; by Prof. Ganin, on the development of fishes; and by 
M. Sidoroff, on the insects destroying corn in Russia, ‘ 

A most interesting communication was made to the Section of 
Physiology by Prof. Setchenoff, on the absorption of oxygen 
and nitrogen by blood. Besides, we notice communications by 
Prof. Goloubeff, on the vibratile epithelium ; by Dr. Tsiboulsky, 
on a new method of determining the amount of blood in ani. 
mals ; by M. Wedensky, on the innervation of the respiratory 
motions of the Rana temporaria ; and by Prof. Tarkhanoff, on 
the amount of blood of man, 


‘ ) M. Severtsoff | 
gave a very interesting lecture on the orographical structure of | 
Central Asia and on its influence upon the geographical distribu- | 








In the Section of Anthropology were the following commu- 
nications :—By Prof. Stid (Dorpat), on the relation between 
the indexes of the skull and that of the head ; by Dr. Lubinsky 
on the sight, being the result of numerous observations upon the 


| crews of the Russian navy, which observations establish a cer- 


tain connection, difficult to explain, between the power of sight 
and the breadth of the chest, The communication by M. 
Dokouchaeff, on the pre-historic man of the downs of the Oka 
river, deals with a subject of great interest, as he affirms that 
the range of downs which we see along the whole of the course 
of that river must afford a great amount of pre-historic remains, 
as is the case with the downs of Volosovo and Lviniy, both 
having yielded thousands of such remains. Prof. Inostrantseff 
discussed at length the various sub-divisions of the stone period, 
and M. Anoutchin gave an interesting note on the frontal 
suture, which seems to appear most frequently in races of a 
higher degree of civilisation, 

An interesting feature of these Russian congresses is the 
existence of two special sections, those of scientific medicine and 
of hygiene ; the latter section has assumed a great importance, 
thanks to the energy of several eminent hygienists, as Drs. 
Erisman, Dobroslavine, Vyrouboff, and others. A question 
being raised about the hygiene of railways, the section of hygiene 
had two special sittings on this subject, and a committee was 
appointed to draw up a programme of investigations on the 
dress of railway employés, the number of hours of work, 


L | the sanitary state of railway stations, and of dwellings of 
In the Section of Astronomy and Mathematics we notice the | 


employés, accidents, the transport of cattle, &c. A great number 
of other questions, as to the disinfection of dwellings, epidemics, 
&c., were discussed, and we hope that the work of the section 
will be of great importance for this kind of investigation. 
Several other important communications were made in the 
Physical Society, and in the St. Petersburg Society of Naturalists. 
which both have had their annual meetings during the Congress. 





UNIVERSITY AND EDUCATIONAL 
INTELLIGENCE 
Oxrorp.—On February 3 the question of the Natural Science 
Last 
term, it will be remembered, the proposal to grant a special 


| natural science degree was defeated after a close division, the 


principal opposition to the motion coming from the scientific 
members of congregation. It was thought that a separate 
science degree, not carrying with it the privileges of the master 
of Arts Degree, would be regarded as an inferior degree, and tend 
to lower the position of science in the University. A clause is 
now proposed by an influential body of residents—including 
Prof. Odling, Dr. Mark Pattison, Rector of Lincoln, A. Vernon 
Harcourt, Prof, Green, Prof. Lawson, and Prof, Nettleship—to 
the following effect:—‘‘ Every person who shall have been 
admitted to the degree of Master of Natural Science, shall also 
be admitted to the degree of Master of Arts.” 

At the University Museum Prof, Clifton will continue his 
course on Statical Electricity and Magnetism ; Dr, Odling will 
continue his lectures on Organic Chemistry on Mondays and 
Fridays at noon, instead of on Mondays and Thursdays as here- 
tofore. The examination for the Radcliffe Travelling Fellow- 
ship will begin in the Museum on Tuesday, February 10, at 
10 A.M. Candidates are requested to send in their names to Dr. 
Acland, at the Museum, on or before February 1. 

At Christ Church Mr. Vernon Harcourt will form a class and 
lecture on Quantitative Analysis; Mr. Baynes will lecture on 
Thermodynamics and Electrodynamics, 


M. Roucet, Professor of Physiology in the Faculty of Medi- 
cine at Montpellier, is nominated Professor of General Physiology 
in the Museum of Natural History of Paris, in succession to the 
late Claude Bernard. 





SCIENTIFIC SERIALS 


Annalen der Physik und Chemie, No. 12, 1879.—Analogies 
between fluidity and galvanic conductivity, by O. Grotrian.—On 
the magnetisation of iron rings, by A. v. Ettingshausen. —The ball- 
shaped electro-dynamometer, by J. Fréhlich.—On gradual passage 
of the band-spectrum of nitrogen into a line-spectrum, by A, 
Wiillner.—On Stokes’s law, by S. Lamansky.—On a bi-constant 
dispersion formula, by E. Lommel.—On the dichroitic fluores- 
cence of magnesium-platinum-cyanide ; experimental proof of 





290 


NATURE 


[ Fan. 22, 1880 





the perpendicularity of the light vibrations to the plane of 
polarisation, by E. Lommel.—On a small alteration of the 
Bunsen grease-spot photometer, by A. Toepler.—On the refrac- 
tion of sound-waves, by K. W. Schellbach and E, E, Boehm.— 
On the specific heat of water according to Dr. Baumgartner’s ex- 
periments, by L. Pfaundler.—Reply to the observation of O. E. 
Meyer, by L. Boltzmann.—On the application of the telephone 
to measurements of resistance, by F, Niemdller.—On the motion 
of glaciers, by K. R. Koch and F. Klocke.—On hailstones with 
ice-crystals, by Ed. Hagenbach.—On hailstones of uncommon 
size, by P. Merion. (In a paper prefixed to this number, Prof. 
Clausius defends himself against some aspersions, by Herr 
Diihring, regarding'his relations to Robert Mayer, @ propos of the 
mechanical theory of heat.) 


THE Sitzungsberichte der naturwissenschaftlichen Gesellschaft 
Jsis in Dresden (1879, January to June) contain the following 
papers of interest :—On the recent geographical and geological 
investigations of the United States of America, by Dr. Geinitz. 
-—On the coal flora of the Lugan coal-pits, by H. Krone.—On 
the constitution of dichlornitrophenol, by Dr. Schmidt.—On a 
new form of the influence machine, by Dr. Tépler.—On the 
action of chloride of lime upon absolute alcohol, by Dr. Gold- 
berg. —On a gas-stove with arrangement for oxidation, by Dr. 
Hempel.—On a new dye, by Dr. Schmitt.—On the isomerism 
of ethanes, by Dr. Goldberg.—On the tension of threads and 
Poggendorff’s fall machine, by Dr. Amthor,—On a discovery 
from the later stone period made in Bohemia, by W. Osborne 
(with 5 plates),—On the prehistoric centres of culture in Schles- 
wig, by Herr Michelsen,—On some objects found by Dr. Schlie- 
mann in his excavations in Greece and Asia Minor, by Dr. 
Fiedler.—On a discovery of urns at the Hradischt, near Stra- 
donic (Bohemia), by W. Osborne.—On the occurrence of Cas- 
tanea vesca, L., by Dr. Friedrich.—Various smaller botanical 
papers of minor interest.—On the theory of Watts’s centrifugal 
regulator, by Dr. Ritterhaus.—On some galvanometric methods 
of multiplication, by Dr. Tépler.—Remarks on Wallengren’s 
work concerning Linnzeus’s species of the genus Phryganea, by 
M. Rostock.—On the Neuroptera of Saxony, by the same; a 
most elaborate treatise with complete list and catalogue.—On 
the Hemiptera fauna of Transcaucasia, by Dr. von Horvath._— 
Obituary notices of Dr, Eduard Lésche and H. G. Ludwig 
Reichenbach. 


Reale Istituto Lombardo di Scienze e Lettere, vol. xii. fase. 
xvii.-xviiii—This number contains a survey of the year’s work, 
announcements of prizes awarded (wi-h abstracts of memoirs), 
and of prize subjects, &c. 

Fasc. xix.—Stratigraphic observations on the precarboniferous 
formation of Valtellina and Calabria, by S. Taramelli.—On the 
dilatation of the heart in disorders of the ventricle, by Prof, de 
Giovanni. 

Fournal de Physigue, December, 1879.—We note here the 
following :—Measurement of the wave-length of obscure calorific 
rays, by M. Mouton.—Displacement between oxygen and the 
halogen elements united with metals, by M. Berthelot.—A 
spectroscope for studying the phenomena of fluorescence, by M. 
Lamansky. 

Journal of the Franklin Institute, December, 1879.—On a 
new theory of the retaining wall, by Prof. Du Bois.—A system 
of electrical storage, by Professors Houston and Thomson,— 
Steam boiler explosions, by Messrs. Corbin and Goodrich. 





SOCIETIES AND ACADEMIES 
LONDON 

Royal Society, January 15.—‘‘ On Chemical Repulsion,” by 
Edmund J. Mills, D.Se., F.R.S. 

While engaged in some researches on the propagation of 
chemical change, I have incidentally encountered a new order of 
phenomena, which the title ‘‘chemical repulsion” may serve 
provisionally to designate. A brief outline of the experiments is 
given in the following paragraphs. 

Upon a glass plate, laid in a horizontal position, is poured 
enough solution of baric chloride to cover it canning to a 
considerable depth. On this solution is placed another glass 
plate, provided with a small central perforation; when the two 
plates are firmly pressed together with the hands, most of the 
solution is extruded, and only a very thin layer of it left between 
the plates. All excess of the solution having been removed 
from the outer surfaces of the plates as well as from the perfora- 





tion, some dilute hydric sulphate is now introduced into the 
perforation. This reagent attacks the baric chloride, throwing 
down a white precipitate of sulphate ; and, proceeding partly by 
diffusion, partly by flow, does not cease to widen in every direc- 
tion its figure of advance, until the edges of the plates are 
attained. If the perforation is circular, the figure of advance is 
pt in other words, the chemical development of a circle is 
a circle, 

Let us now suppose the two plates to be square and equal, and 
let the upper one have two circular perforations, equidistant 
from the centre of the square, and situated upon its diagonal. 
Let also two circular developments of baric sulphate be caused 
to proceed, as before, from the two perforations simultaneously, 
At first nothing remarkable is observed, but in a short time, the 
two growing circles begin to exercise a visible retardation on 
each other’s progress ; so that the figure of advance is no longer 
circular, but oval, [This retardation is of course observed only 
between the perforations; and not outside them, where the 
motion is entirely free.] As the development of the fizures 
continues, so also does the retardation at their neighbouring 
edges increase ; the final result being (however long the experi- 
ment may be prolonged), that the other diagonal of the square 
is completely and permanently traced out in a line of no chemical 
action. 

The above experiments are of fundamental importance, and 
they obviously adinit of endless variety. Of this, a few illustra- 
tions may suffice. 

If the upper plate have three perforations, situated on the 
points of a central equilateral triangle, there are three repulsion 
lines ; these end at the centre of the triangle, where they form 
a trilocular point, and traverse its sides midway at right angles. 

When the upper plate has four perforations, situated on the 
points of a central square, there are four, repulsion lines; these 
end at the centre of the square, where they form a quadrilocular 
point, and traverse its sides midway at right angles, 

A very beautiful modification of the preceding experiment 
consists in simultaneously developing a circle from a (fifth) 
central perforation, This last circle has no means of escape 
from the surrounding four. The result is, that it eventually 
forms a square figure bounded by repulsion lines, and having 
four symmetrically situated repulsion lines at its corners. 

It is easy to demonstrate that the chemical repulsion in these 
experiments does not depend upon flow. Two superimposed 
triangular plates, for instance, in neither of which is any perfora- 
tion, give three repulsion lines on immersion in dilute hydric 
sulphate. From each corner a line proceeds midway (if the 
triangle be equilateral) to the centre. In this effect diffusion is 
alone concerned. 

In addition to hydric sulphate and baric chloride, other pairs 
of reagents may be used with success ; and I anticipate no diffi- 
culty in obtaining results in which precipitation is not concerned. 
A beginning has also been made with experiments in tridimen- 
sional development. 

The complete explanation of what I have termed ‘‘ chemical 
repulsion” will probably demand a varied and considerable 
amount of experimental work. From some incidents of the 
investigation, so far as it has hithert> proceeded, I am disposed 
to believe that the motion in any plane chemical figure is not 
along the radius, but at right angles to the radius ; and this sup- 
position will, if verified, explain the repulsion. The existing 
results afford proof of the following propositions, viz. :— 
(1) Chemical action can take place at a distance ; and (2) Two or 
more chemical actions, identical except in position, completely 
exclude one another. 


Chemical Society, January 15.—Mr. Warren De La Rue, 
president, in the chair.—The following papers were read :—On 
the effects of the growth of plants on the amount of matter 
removed from the soil by rain, by Dr. J. H. Prevost. Soil 
3 inches deep was placed in two glazed earthenware pans 
17 inches in diameter on July 21 ; 4 grm. of white clover seed 
was sown in one, the other being blank. The pans were 
exposed till October 4. The drainage-water was collected and 
analysed ; that from the clover soil contained 48*1 grains of solid 
matter per gallon, the other 220, The author concludes that 
rain removes much more matter from an uncropped than from @ 
cropped soil.—Mr. Wynter Blyth described a simple apparatus 
for the treatment of substances in open dishes to volatile solvents. 
The dish is placed inside a cast-iron pan, and covered with a 
glass bell-jar, with condenser attached, the joint between the 
bottom of the pan and the bell-jar being made tight with 





Fan. 22, 1880] 


NATURE 


291 





mercury.—On dibromanthraquinones, by Mr. W. H. Perkin. By 
heating bromine with anthraquinone, a dibromanthraquinone 
is formed, melting at 245°C. ; by boiling tetrabromanthracen with 
chromic acid, dissolved in’a large excess of glacial acetic acid, an 
isomer 8 dibromanthraquinone is obtained, melting at 275° C. 
By the action of caustic alkalies on these bodies, alizarin is formed 
in both cases, The author discusses the formation of this 
substance, In the case of the a body, two other colouring 
matters were formed with the alizarin, one dyeing mordants, the 
other not. The author is investigating these bodies. He 
appends a note in which he concludes on further examination 
that Auerbach’s isopurpurin is a mixture of flavopurpurin and 
anthrapurpurin, and is not identical with anthrapurpurin.—Mr. 
Warington contributed some notes on some practical points 
connected with his laboratory experience. He has used with 
great convenience the indiarubber joint covered with mercury, 
which was proposed by Dr, Frankland as a substitute for the 
steel blocks connecting the laboratory and measuring tubes. At 
first the indiarubber wore out rapidly ; this was prevented by 
tying it above the conical stopper as well as below He re 
commends the coating of laboratory benches, &c., by heating the 
wood and then rubbing in paraffin; the wood is thus protected 
from the action of acids. In the determination of nitrates by 
Frankland’s process, the author suggests the addition of a drop of 
dilute hydrochloric acid, to ensure a complete reaction between 
the mercury and the nitric acid. By means of a solution of 
diphenylamine in strong sulphuric acid, the author has detected 
by the blue coloration produced yyjysth of a milligram of 
hydrogen as nitric acid.—On the melting and boiling points of 
certain inorganic substances, by T. Carnelly and W. C. Williams. 


Zoological Society, January 6.—Prof. Flower, F.R.S., 
president, in the chair.—Prof. Newton, M.A., F.R.S., V.P., 
exhibited, on behalf of Mr. G. B. Corbin, a speciwen of Acan- 
thyllis (sive) Chetura caudacuta, the Needle-Tailed Swift, shot 
near Ringwood, in Hampshire, in July, 1879, remarking that it 
was the second example of this Siberian species which had been 
obtained in England.—Mr, John Henry Steel, F.Z.S., read a 
series of preliminary notes on the individual variations observed 
in the osteological and myological structure of the Domestic Ass 
(Zquus asinus).—A communication was read from Mr, E, W. 
White, C.M.Z.S., containing notes on the distribution and 
habits of Ch/lamyphorus truncatus, from observations made by 
the author during a recent excursion into the western provinces 
of the Argentine Republic, undertaken for the purpose of ob- 
taining a better knowledge of this animal.—Dr. John Mulvany, 
R.N., read a paper on a case which seemed to him to indicate 
the moulting of the horny beak in a Penguin of the genus 
Endyptts.—Mr. O. Thomas, F.Z.S., read the description of a 
new species of MZus, obtained from the island of Ovalau, Fiji, 
by Baron A, von Hiigel, and proposed to be called Mus huegeli 
after its discoverer.—A communication was read from Mr. R. 
G, Wardlaw Ramsay, F.Z.S., containing a report on a collec- 
tion of birds made by Herr Bock, a naturalist employed by the 
late Lord Tweeddale, in the neighbourhood of Padang. Three 
species were described as new and proposed to be called Dicrurus 
sumatranus, Turdinus marmoratus, and Myiophoneus castaneus. 
—Dr. Giinther, F.R.S., read adescription of two new species 
of Antelopes, of the genus Meotragus, N. hirki, from Eastern 
Africa, and NV. molaris, from Damaraland. 


Geological Society, January 7.—Henry Clifton Sorby, 
president, in the chair.—Edward Bagnall Poulton was elected a 
Fellow, and Prof. A. E. Nordenskjold, Stockholm, and Prof. 
F, Zirkel, Leipzig, Foreign Members of the Society.—The 
following communications were read :—On the Portland rocks 
of England, by the Rev. J. F. Blake, F.G.S. The author gave 
a general account of the relation of the several Portland rocks 
in the areas of their development to each other, and hence de- 
duced the history of the Portland ‘‘episode.” The name is 
used on the Continent in a wider sense than in England, and 
this use was shown to be unjustifiable. After giving an account 
of his observations on the rocks at Portland itself, and dividing 
the limestones into the building-stone and flinty series, the author 
showed that the so-called ‘‘ Upper Portlandian” of Boulogne 
corresponds to the latter, and the upper part of the ‘Middle 
Portlandian” to the Portland sand, He then endeavoured to 
prove, by the proportionate thickness, the indications of change 
in the lithology, and the distribution of some of the fossils, that 
ae ae, of the ——— ‘ Middle” and the ‘‘ Lower Port. 

I "are represent y integral portions of the Upper 
Kimimeridge, which are thus the “‘ oly ” form cortenponiing 





to what the author calls the ‘‘ Boulognian episode.” The series 
in the Vale of Wardour has been made out pretty completely. 
The Purbeck is separated by a band of clay from the Portland, 
and is not amalgamated with it. The building-stones and flinty 
series are here seen again; and a fine freestone occurs at the 
base of the latter. The representatives of the Portland sand 
were considered to be older than those of other districts. The 
relations of the Purbeck to the Portland rocks at Swindon were 
very carefully traced; and it is shown that, while the upper 
beds ‘of the latter put on here some peculiar characters, the 
former lie on their worn edges. The upper beds of the Port- 
land, which have been referred to the sand, correspond to the 
freestone and the base of the flinty series of the Vale of War- 
dour ; hence the Purbecks of Swindon may be coeval with the 
upper beds of the Portland to the south. At the base of the great 
quarry and elsewhere in the neighbourhood are the ‘‘ 7rigonia- 
beds,” beneath which is clay, hitherto mistaken for the Kimmer- 
idge clay ; and beneath this are the true Portland sands, with 
an abundant fauna new to England. The limestones of Oxford- 
shire and Bucks were considere1 to represent the ** 7rigonia- 
beds ” only; and, as the Purbecks here lie for the most part 
conformably, it was suggested that they were formed ina lake 
at an earlier period than those at Swindon, which are of a more 
fluviatile character. Hence the Portland episode, considered as 
marine, was at an end in the north before it was half completed 
in the south.—On the correlation of the drift-deposits of tke 
north-west of England with those of the midland and eastern 
counties, by D. Mackintosh, F.G.S. 


Anthropological Institute, Jan. 13.—John Evans, D.C.L., 
F.R.S., vice-president, in the chair.—Dr, Hack Tuke read a 
paper on *‘ The Cagots.” The author showed that the popular 
etymology of the word Cagot, from ‘‘ Canis Gothi,” is probably 
inaccurate, and accepted the suggestion of ‘M. de Rochas, that 
Cagot is derived from the Celto-Breton word caced (leprous) ; it 
is easy to see how readily this would assume the form of cacou 
(as it is in Brittany actually applied to these people), and so the 
French Cagou or Cagot. The conclusions at which the author 
arrived as to the origin of the Cagots were as follows:—1. The 
Cagots are not the descendants of the Goths; they are not a 
distinct race, but a despised class among the people of the 
country in which they live. 2. They are not more subject to 
goitre or to cretinism than the inhabitants of the adjacent district 
—in short, cagotism and cretinism are in no way allied. 3. The 
present representatives of the Cagots are now recognised by tradi- 
tion, and not by their features, and are not distinguished by any 
peculiar mental or physical disorder. 4. Although nothing like 
leprosy, or leucoderma, has for a long time affected the Cagots, 
and no one on the spot regards them in this light, there is 
evidence to show that they were originally either lepers labouring 
under a particular variety of leprosy, or were affected with leu- 
coderma, the form of the affection accounting for their being 
regarded as in some respects different from ordinary lepers, 
though shunned in the same way. 5. Many were, no doubt, 
falsely suspected of leprosy in consequence of some slight 
skin affection ; others, again, in later centuries, were members 
of families in which the disease had died out.—The Director 
read two papers by Mr. Alfred Simson, on the Jivaros 
and the Canelos Indians, The tribe of the Jivaros is a 
large one, and one of the most distinguished, independent, 
and warlike in South America, They speak a language 
of their own, Jivaro, and occupy the country generally from 
the Upper Pastassa to the Santiago, both rivers included, 
down to the Pongo de Manseriche, on the Marafion. They 
are hospitable, and their houses are large and built of 
palms, They have a most perfect method of scalping, by which 
the victim’s head is reduced to the size of a moderately large 
orange, maintaining tolerably well all the features : the skinis cut 
round the base of the neck, and the entire covering of the skull 
removed in one piece. This is then dried gradually by; means 
of hot stones placed inside it, until the boneless head shrinks to 
the required size. They also wear their slain enemies’ hair in 
long plaits round the waist. Great festivities take place when a 
child, at three or four years of age, is initiated into the art and 
mysteries of smoking. The Jivaros of the Pintue have the 
habit of vomiting nearly every morning by the aid of a feather, 
arguing that all food remaining in the stomach overnight is un- 
wholesome and undigested, and should therefore be ejected. 
Canelos, the once attractive Spanish settlement, but now 
forlorn Indian village, is situated on the left bank of the Bobo- 
naza, one of the most important, if not the largest, of the 





292 


NATURE 


[Fan. 22, 1880 





tributaries of the Upper Pastassa, and is inhabited by a mixed 
tribe of Indians in whom the chief element is Jivaro, though 
some of the better traits of these seem to be wanting in them. 
Their language is Quichua. Their fighting is done entirely with 
the lance, which is their inseparable companion, and all the 
author’s attempts to induce any of them to part with his weapon 
were fruitless. 
PARIS 

Academy of Sciences, January 12,—M. Edm, Becquerel in 
the chair.—M. Daubrée presented the second part of his 
Synthetic studies of experimental geology ; it treats chiefly of the 
chemical and mechanical phenomena of meteorites (which are 
compared with the deeper rocks).—On meteorological observa- 
tions in May at Zi-ka-wei, in China, by M. Faye. Storms go 
from China to Japan, following a like course to that of storms 
coming to Europe from the Atlantic. They are independent of 
the prevailing monsoon, and conversely, neither preventing the 
other. M. Faye finds support for the theory of gyratory move- 
ments propagated downwards.—On the kinematic geometry of 
deformations of bodies, elastic, plastic, or fluids, by M. De Saint 
Venant.—Some observations on a note of M. Wurtz (C. 2., 
December 22, 1879), by M. Sainte-Claire Deville.—Evolution 
of the inflorescence in Graminez (first part), by M. Trécul. He 
considers here (1) the formation of the primary axis; (2) the 
order of appearance of the branches ; (3) that of their growth.— 
Influence of the nature of carbons on the electric light, by M. 
Tu Moncel. In 1855 he called attention to the advantages of 
using carbons of vegetable origin for the electric light. In 1859 he 
produced an electric candle with plates of charcoal in a tube.—On 
the disaccord apparent between the heights recently observed 
on the Seine and the previsions of the hydrometric service in the 
passage through Paris, by MM. Lalanne and Lemoine. M. 
Belgrand’s empirical laws-apply only to the natural state 
of the river, but ceased to apply in the early days of January, 
owing to the effects of the abnormal freezing of the Seine (which 
occurs several times in a century). M. Dumas and Gen. Morin 


made some remarks, the General pointing out that the breaking 
up of the ice sometimes proceeds up the river, sometimes down ; 
in the latter and more dangerous case explosives and other 
means should be promptly used to open the block.—On the 
photographic spectra of stars, by Dr, Huggins.—State of the 


tunnelling operations of St. Gothard, by M. Colladon. The 
works have been retarded. From November 11 to January 1 
(fifty-one days) the advance of the north gallery was only 
3490 m, against 173‘10 m, in the forty-nine days previous, This 
was due to pressure of an unresistant rock met with, which 
crushed the strongest wood-work, The perforation will likely 
be complete in the end of February or beginning of March.—On 
treatment of phylloxerised vines, by M. Marés.—On glyco- 
genesis in infusoria, by M. Certes. Treated with iodised serum, 
they present similar effects to those whereby M. Ranvier, with 
this substance, proved the [ pomeer of glycogen in lymphatic 
cells. (The effects on several organisms found with infusoria are 
also indicated.) The vitality of animalcules is an important 
factor in glycogenesis.—Resistance of pucerons to severe cold, by 
M. Lichtenstein, Phylloxera and others successfully resisted 
cold of 11° and 12° below zero in December.—Determi- 
nation, by M. Gylden’s methods, of the motion of the planet 
Hera (103), by M. Callandreau.—On the polygons inscribed 
in a conic, and circumscribed on another conic, by M. Dar- 
boux.—Solar cyclone, by M. Thollon. Observing a peculiarly 
dark spot on January 3, he perceived two opposite deflections of 
the line C, corresponding to velocities of 60 and 137 km. respec- 
tively, in the vast cyclone.—On the thermal laws of the electrie 
sparks produced by ordinary partial discharges of condensers 
(second note), by M. Villari. The galvanometric deflections caused 
by incomplete discharges are proportional to the quantities of 
electricity forming the discharges. The heat generated by the 
spark is directly proportional to the quantity of electricity 
forming the spark.—Variations of the netic declination 
deduced from regular observations at Montcalieri in the period 
1871-78, by M. Denza. These agree in the main with observa- 
tions at other Italian places, and at Prague, Christiania, Munich, 
and Greenwich, pointing to cosmical causes.—On the Thomson 
galvanometer, by M. Gaiffe. The scale-indications are not pro- 
ee to the values of the currents measured, the angles of de- 

ection of the needle being doubled by reflection of the mirror, 
This source of error he seeks to correct by using a bifilar suspen- 
sion formed of two cocoon-fibres.—On the potash-contained in 
the clay of arable soils, by M. Perrey. Clay constantly contains 





potash varying ordinarily from 2 to 5 per cent., sometimes from 
1°8 to 7°3 per cent.—On the tension of dissociation of hydrate of 
chloral, and on the vapour-tension of anhydrous chloral, by MM, 
Moitessier and Engel.—Effects of intra-venous injections of 
sugar and gum, by MM. Moutard-Martin and Richet. Sugar 
injected into dog’s veins always causes polyuria and glycosuria, 
and does not affect the blood-pressure. Gum has an opposite 
effect ; it diminishes the polyuria iously produced by sugar, 
and at length completely stops the secretion of urine ; it also 
increases notably the tension of blood in the arteries.—On the 
phenomena arising from ligature of :the inferior vena cava above 
the liver, by M. Picard, 


a 


VIENNA 


Imperial Academy of Sciences, October 23, 1879.—The 
earthquakes of Carinthia and their lines of shock, by Prof, 
Hoefer.—On the histiogenesis of sclerosis of the posterior fibres 
of the spinal cord, by Dr. Weiss.—On the forces operative on 
diamagnets, by Prof. Bolzmann.—Determination of path of the 
planet Bertha (154) by Herr Anton, 

November 6, 1879.—The long-haired common guinea-pig 
(Cavia Cobaya longipilis), by Dr, Fitzinger.—Fish-fauna of the 
Cauca and the rivers in Guayaquil, by Dr. Steindachner,— 
Shell-fish fauna of the Galapagos Islands, by Herr Wimmer,— 
The von Miiller collection of Australian fish, by Dr. Klunzinger, 
—On the humour passages of hyaline cartilage, by Dr. Spina. 
—Magnetic measurements in Kremsmiinster in July, 1879, by 
Herr Liznar.—On compounds from animal tar: III. Lutidine, 
by Prof. Barth and Herr Herzig. 

November 13, 1879.—Researches on the development of the 
central nerve-tissue, by Herr Stricker and Dr. Unger.—On the 
action of the safety- valve in steam boilers, by Herr von Burg.— 
Firing under water, by Herr Lorber. 

November 20, 1879.—The following among other papers were 
read :—The sporogon of Archidium, by Prof. Leitgeb,—Con- 
tributions to a knowledge of the hen’s germ at the commencement 
of brooding, by Herr Koller.—On the last multiplier of differ- 
ential equations of higher order, by Prof. Winckler. 

December 4, 1879.—On the striction line of the hyperboloid 
as rational space-curve of fourth order, by Herr Migotti.—On 
processes of degeneration and regeneration in uninjured peripheric 
nerves, by Prof. Mayer. 

December 11, 1879.—On waterspouts observed near Canea, 
by Herr Miksche.—Researches on the course of conduction in 
the spinal cord of the dog, by Dr. Weiss.—A contribution to 
the theory of urine-secretion, by Dr. Gartner.—On a new isomer 
of gluconic acid, by Herr Hénig.—On the theory of inconstant 
galvanic elements, by Prof, Exner. rw 





CONTENTS Pace 


On THE PxHorocrapnic Spectra oF Stars. By W. Huacns, 
D.C.L., LL.D., F.R.S. (With [ilustrations) a 
Vocat Puysiotocy AND Hycriene. By Dr. Wiit1aM Po g, F.R.S. 
Tue Coprer-Tin ALtoys. By W. CHANpDtER Roserts, F.R.S.. . 

Our Boox SHEuF :— 
Pickard-Cambridge’s ‘Spiders of Dorset, with an Appendix con- 
taining Short Descriptions of those British Species not yet found 

irr Dorsetshire ”’ 


Causes, and the Means of Preventing them” . . . 
LetTers TO THE EDITOR :— 

Ice-Crystals.—The Duxe of ARGytL. . . . 2 2 se eo 
Re-Reversal of Sodium Lines.—C, A. YounG .... + « 
Death of Capt. Cook.—Rosert Mauuet, F.R.S. . . 2. 2 + + 
Electricity of the Blowpipe ‘‘ Flame.”—Col. W. A. Ross 
Suicide of Scorpion.—F. GittMan *) « 
The Fertilisers of Alpine Flowers.—Dr. HERMANN MOLLER . - 
“ Tdeal’’ Matter.—Percy R. HARRISON . . 


Sun-Spots.— Henry Beprorp} . . 4 

A Clever Spider.—Li. A. MorGAN . . « « + 2 «© « = 

Erratum in Paper on Tidal Friction. —G. H. Darwin, F.R.S. . 
ArGHaN Erunotocy. By A. H. Keane . . 
Tue Mereoro.ocy or SourH AUSTRALIA. .- 
AlcGe... . 
Gas AND Ex . 
ROUER os vow: wie ee ele . . 
Our Astronomicat CoLtumN:— 

The Orion-Trapezium . 

The Total Solar Eclipse 
Grotocicat Nores 
Puysicau Norss . 


Geocrapuicat Nores . . + ++ + + # « + 
Tue Stxtu Concress or Russian NATURALISTS 
University aND EpucaTIONAL INTELLIGENCE . 
Screntiric SerIAts . «. - 
SocreTtss AND ACADEMIES